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Large self-illuminated object in space
form of a white dwarf. Intermediate-mass stars, between ~2.25 M☉ and ~8 M☉, pass through evolutionary stages similar to low mass stars, but after a relatively
Star
Class of black holes with a mass range of 100 to 100000 solar masses
An intermediate-mass black hole (IMBH) is a class of black hole with mass in the range of one hundred to one hundred thousand (102–105) solar masses: significantly
Intermediate-mass_black_hole
Topics referred to by the same term
Intermediate mass may refer to: An intermediate-mass black hole, a black hole with a mass between 102 and 105 solar masses An intermediate-mass star,
Intermediate_mass
Class of binary stars
classification by mass (high, intermediate, low) refers to the optically visible donor, not to the compact X-ray emitting accretor. Low-mass X-ray binaries
X-ray_binary
Spherical collection of stars
black holes at their centers. The mass of these supposed intermediate-mass black holes is proportional to the mass of their surrounding clusters, following
Globular_cluster
Compact astronomical body
supermassive black holes, are rarer than either extreme, and are called intermediate-mass black holes. Physicists have speculated that such black holes may
Black_hole
Type of star, larger and brighter than the Sun
eventually become a supernova. Stars in the 8~12 M☉ range have somewhat intermediate properties and have been called super-AGB stars. They largely follow
Giant_star
Two pulsars orbiting each other
same. Subsequent observations continue to show this decrease. An intermediate-mass binary pulsar (IMBP) is a pulsar-white dwarf binary system with a
Binary_pulsar
Galaxy containing the Solar System
2019. Watkins, Laura L.; et al. (February 2, 2019). "Evidence for an Intermediate-Mass Milky Way from Gaia DR2 Halo Globular Cluster Motions". The Astrophysical
Milky_Way
List of some black holes
List of quasars List of nearest black holes Supermassive black hole Intermediate-mass black hole Stellar black hole Micro black hole Lists of astronomical
List_of_black_holes
Closest known white dwarf star to Earth
Major or the "Greater Dog". It is a white dwarf, a remnant of an intermediate-mass star that has exhausted its fuel, and is the closest example to Earth
Sirius_B
possible way for an intermediate mass ratio inspiral is for an intermediate mass black hole in a globular cluster to capture a stellar mass compact object
Extreme_mass_ratio_inspiral
European space mission to measure gravitational waves
able to detect events up to redshifts around 1. In the case of an intermediate mass black hole spiralling into a massive black hole (between 104 and 106
Laser Interferometer Space Antenna
Laser_Interferometer_Space_Antenna
Binary Star in the constellation Hercules
falls on the borderline, ~2 M☉, between high- and low-mass X-ray binaries. An intermediate-mass X-ray binary (IMXB) is a binary star system where one
Hercules_X-1
Type of large cool star
absolute magni- tude (MV) A red giant is a luminous giant star of low or intermediate mass (roughly 0.3–8 solar masses (M☉)) in a late phase of stellar evolution
Red_giant
Band of tissue connecting the two halves of the thalamus
The interthalamic adhesion (also known as the massa intermedia, intermediate mass or middle commissure) is a flattened band of tissue that connects both
Interthalamic_adhesion
Globular cluster in the constellation Centaurus
core remnant of a disrupted dwarf galaxy. There is evidence of an intermediate-mass black hole in the dense core of this cluster, although this is disputed
Omega_Centauri
Portion of the giant branch before helium ignition
evolution. It is a stage that follows the main sequence for low- to intermediate-mass stars. Red-giant-branch stars have an inert helium core surrounded
Red-giant_branch
Radius of the event horizon of a Schwarzschild black hole
Yuhei; Tsujimoto, Shiho; Nomura, Mariko (2019). "Indication of Another Intermediate-mass Black Hole in the Galactic Center". The Astrophysical Journal. 871
Schwarzschild_radius
Edmund; Horst, John C. (2021-11-01). "Hα Reverberation Mapping of the Intermediate-mass Active Galactic Nucleus in NGC 4395". The Astrophysical Journal. 921
List of most massive black holes
List_of_most_massive_black_holes
Subatomic particles
thermal temperature of the emitting medium. In the intermediate-mass region (IMR), with invariant mass above about 1 GeV, hadronic resonance contributions
Dilepton
Star at the centre of the Solar System
P. R. (1993). "Evolution of low- and intermediate-mass stars to the end of the asymptotic giant branch with mass loss". The Astrophysical Journal. 413:
Sun
Type of star that is massive and luminous
stars of intermediate mass that have particularly low surface gravities, often due to instability such as Cepheid pulsations. These intermediate-mass stars'
Supergiant
Type of x-ray source
powers ULXs; models include beamed emission of stellar mass objects, accreting intermediate-mass black holes, and super-Eddington emission. ULXs were first
Ultraluminous_X-ray_source
Type of emission nebula created by dying red giants
used. All planetary nebulae form at the end of the life of a star of intermediate mass, about 1-8 solar masses. It is expected that the Sun will form a planetary
Planetary_nebula
Collapsed core of a massive star
star Intermediate-mass X-ray binary pulsars: a class of intermediate-mass X-ray binaries (IMXB), a pulsar with an intermediate mass star High-mass X-ray
Neutron_star
Type of star larger than main-sequence but smaller than a giant
classes. The subgiant branch is a stage in the evolution of low to intermediate mass stars. Stars with a subgiant spectral type are not always on the evolutionary
Subgiant
Grouping of evolved cool luminous stars
This is a period of stellar evolution undertaken by all low- to intermediate-mass stars (about 0.5 to 8 solar masses) late in their lives. Observationally
Asymptotic_giant_branch
Hot, giant star of early spectral type
horizontal branch, intermediate-mass stars that have passed through a red giant phase and are now burning helium in their cores. Depending on mass and chemical
Blue_giant
Intermediate mass black hole candidate located in the lenticular galaxy ESO 24349
is an intermediate-mass black hole candidate located in the lenticular galaxy ESO 243-49 about 290 million light-years from Earth. The mass of its central
HLX-1
Hypothetical early-universe star with a black hole core
dissipate without a supernova, leaving behind an intermediate-mass black hole. These intermediate-mass black holes are theorized as the progenitors of
Quasi-star
Type of luminous supergiant star
post-asymptotic giant branch) is a type of luminous low-mass supergiant star of intermediate mass in a very late phase of stellar evolution. The post-AGB
Post-AGB_star
Flow of gas ejected from the upper atmosphere of a star
the later stages of evolution. The influence can even be seen for intermediate mass stars, which will become white dwarfs at the ends of their lives rather
Stellar_wind
Natural physical entity in space
luminosity of stars, which allowed them to predict their temperature and mass. In 1913, the Hertzsprung–Russell diagram was developed by astronomers Ejnar
Astronomical_object
American astrophysicist
(HST-GO-9099) that discovered the first, and as yet the only confirmed, intermediate mass black hole in the Globular cluster, G1 in M31. Rich has over 450 refereed
R._Michael_Rich
Hypothetical invisible cosmic material
100% of dark matter in specific mass windows (e.g., evaporating tiny black holes or monochromatic intermediate-mass populations). However, those constraints
Dark_matter
Galaxy in the constellation Ursa Major
Astronomers have postulated that this comes from the first known intermediate-mass black hole, of roughly 200 to 5000 solar masses. M82, like most galaxies
Messier_82
Gravitational-wave event detected in 2023
hole mass gap. GW231123 was the result of the merger of a 137+22 −17 M☉ black hole and a 103+20 −52 M☉ black hole creating a new intermediate-mass black
GW231123
Brightest star in the constellation of Carina
indicates that it is currently in the core-helium burning phase. It is an intermediate mass star that has left the red-giant branch before its core became degenerate
Canopus
Galaxy in the constellation Canes Venatici
of just 4,000 M☉ to 20,000 M☉. The low-mass black hole in NGC 4395 would make it a so-called "intermediate-mass black hole". The black hole may have a
NGC_4395
Stellar classification
surface, and these are the most luminous stars that exist. Low to intermediate-mass stars age in a very different way, through red giant, horizontal branch
O-type_star
Molecular cloud
velocity dispersion was once thought to be due to an intermediate-mass black hole (IMBH) with a mass of about 100,000 solar masses. However, observations
CO−0.40−0.22
Intermediate-mass binary pulsar
J2222−0137 is a nearby intermediate-mass binary pulsar at a distance of 267+1.2 −0.9 pc (approximately 870 light-years), whose low-mass neutron star's companion
PSR_J2222−0137
Black hole formed by a collapsed star
holes, which are much more massive than stellar black holes. They are intermediate-mass black holes (in the center of globular clusters) and supermassive
Stellar_black_hole
Nebula surrounding a dying star
second-from-the-last high-luminosity evolution phase in the life cycle of intermediate-mass stars (1–8 M☉). The name protoplanetary nebula is an unfortunate choice
Protoplanetary_nebula
Body of interstellar clouds
high-luminosity evolution phase in the life cycle of intermediate-mass stars (1–8 M☉). A supernova occurs when a high-mass star reaches the end of its life. When nuclear
Nebula
Continuous band of stars that appears on plots of stellar color versus brightness
convection. Intermediate-mass stars such as Sirius may transport energy primarily by radiation, with a small core convection region. Medium-sized, low-mass stars
Main_sequence
Instrument for conducting a spectrographic survey of distant galaxies
largest number of dwarf galaxies including 2,800 black holes (300 intermediate-mass black holes and 2,500 active black holes) from the EDR. DESI unveiled
Dark Energy Spectroscopic Instrument
Dark_Energy_Spectroscopic_Instrument
Stage of stellar evolution
2019-05-20. Retrieved 2019-01-17. Xu, H. Y.; Li, Y. (2004). "Blue loops of intermediate mass stars . I. CNO cycles and blue loops". Astronomy and Astrophysics
Blue_loop
Globular cluster in Scorpius
for an intermediate-mass black hole (even if an unusually compact cluster of compact objects like white dwarfs, neutron stars or stellar-mass black holes
Messier_4
Curve on the Hertzsprung-Russell diagram representing stars of a particular age
on the HR diagram throughout their life. Newborn stars of low or intermediate mass are born cold but extremely luminous. They contract and dim along
Stellar_isochrone
Star that has a supergiant luminosity class, with a spectral type of F or G
Classical Cepheid variables with periods around ten days and longer. Intermediate mass stars leave the main sequence by cooling along the subgiant branch
Yellow_supergiant
Star in the constellation Musca
protoplanets, thus it is considered an important evolutionary precursor to intermediate-mass stars with multiple super-jovian planets at moderate/wide separations
HD_100546
Group of stars in the constellation Andromeda
Mayall II is considered to have twice the mass of Omega Centauri, and may contain a central, intermediate-mass (~ 2×104 M☉) black hole. It was first identified
Mayall_II
Galaxy in the constellation Ursa Major
source at the nucleus. The brightest of these is consistent with an intermediate-mass black hole accreting matter. The galaxy is also emitting a diffuse
Messier_108
Amount of matter present in an object
In physics, mass is an intrinsic positive physical quantity of a body, which measures its resistance to acceleration. In modern physics, it is generally
Mass
Hypothetical black hole formed soon after the Big Bang
supermassive black holes at the center of massive galaxies, as well as of intermediate-mass black holes. Primordial black holes belong to the class of massive
Primordial_black_hole
Globular cluster in Sagittarius
a team of astronomers reported that they had found evidence of an intermediate-mass black hole in the core of M54. Previously thought to belong to the
Messier_54
Isotope of uranium
with slow neutrons is greater. A fission chain reaction produces intermediate mass fragments which are highly radioactive and produce further energy
Uranium-235
Stellar core remnant
After the hydrogen-fusing period of a main-sequence star of low or intermediate mass ends, such a star will expand onto the red giant branch, and eventually
White_dwarf
Gravitational-wave observation
resulting black hole had a mass equivalent to 142 times that of the Sun, making this the first clear detection of an intermediate-mass black hole. The remaining
GW190521
Branch of astronomy using gravitational waves
Ground-based detectors could potentially detect binaries containing an intermediate mass black hole of several hundred solar masses. Supermassive black hole
Gravitational-wave_astronomy
Theoretical cosmological structure
; Sohn, Sangmo Tony; Wyn Evans, N. (2019-03-12). "Evidence for an Intermediate-mass Milky Way from Gaia DR2 Halo Globular Cluster Motions". The Astrophysical
Dark_matter_halo
Group of galaxies that includes the Milky Way
James C.; Patterson, Richard J.; Wolf, Joe (2018). "Evidence for an Intermediate-Mass Milky Way from Gaia DR2 Halo Globular Cluster Motions". The Astrophysical
Local_Group
Minor constellation in the southern sky
75,000 light-years. Located in the galaxy ESO 243-49 is HLX-1, an intermediate-mass black hole—the first one of its kind identified. It is hypothesized
Phoenix_(constellation)
Open cluster within the Rosette nebula, in the constellation Monoceros
that otherwise would form low-mass stars or intermediate mass stars. The study also found a low disk fraction for low-mass objects of 39%±9% for objects
NGC_2244
Eddington limit of a neutron star or stellar black hole? Are they due to intermediate-mass black holes? Some ULXs are periodic, suggesting non-isotropic emission
List of unsolved problems in astronomy
List_of_unsolved_problems_in_astronomy
Process of creating new atomic nuclei from existing nucleons
was the most important discovery in nucleosynthesis theory of the intermediate-mass elements since Hoyle's 1954 paper because it provided an overarching
Nucleosynthesis
Subatomic particle
now known with the intermediate mass, the more general term meson was adopted to refer to any such particle within the correct mass range between electrons
Muon
Young stars of spectral types A and B
Sargent (2000) High-resolution studies of gas and dust around young intermediate-mass stars: II. observations of an additional sample of Herbig Ae/Be systems
Herbig_Ae/Be_star
Globular cluster in the constellation Ophiuchus
core region. It is hypothesized that this cluster may be host to an intermediate mass black hole (IMBH) – it is considered well-suited for searching for
Messier_62
Topics referred to by the same term
a gene in humans that encodes the H2.0 homeobox protein HLX-1, an intermediate-mass black hole Hapag-Lloyd Express, a former German airline HLX (game)
HLX
Mass of a star in astronomy
Low-mass stars with a mass below about 1.8–2.2 M☉ (depending on composition) do enter the AGB, where they develop a degenerate helium core. Intermediate-mass
Stellar_mass
Luminosity–temperature relationship in stars
sequence, with limited observable PMS evolution. At the end of a low- or intermediate-mass star's life, the star follows an analogue of the Hayashi track, but
Hayashi_track
Topics referred to by the same term
formed by a collapsed star Intermediate-mass black hole, a class of black hole Supermassive black hole, a black hole with mass above 10⁵ solar masses, usually
Black_hole_(disambiguation)
Double star in the constellation Aquarius
has an extragalactic origin. This star belongs to a group of three intermediate mass stars with a space velocity that is carrying them perpendicular to
Beta_Aquarii
Second brightest star in the constellation Sagittarius
Dodson-Robinson, Sarah (2016-08-01). "The Close Companion Mass-ratio Distribution of Intermediate-mass Stars". The Astronomical Journal. 152 (2): 40. arXiv:1604
Sigma_Sagittarii
Interstellar gas cloud in the Milky Way
25 light-years from Sagittarius A*. It likely hosts an intermediate-mass black hole with a mass of 32,000 times that of the Sun. HCN−0.009−0.044 has a
HCN−0.009−0.044
Indian astrophysicist
specific approach for observing an elusive class of black holes called intermediate-mass black holes. In 2016, he was part of the delegation that met with
Karan_Jani
Contraction of an astronomical object due to the influence of its gravity
Bloecker, T. (May 1995). "Stellar evolution of low and intermediate-mass stars. I. Mass loss on the AGB and its consequences for stellar evolution"
Gravitational_collapse
Galaxy in the constellation Virgo
Point Sources Found to Be Abundant in Low-mass, Late-type Galaxies Predicted to Contain an Intermediate-mass Black Hole". The Astrophysical Journal. 923
NGC_4470
Globular cluster in the constellation Tucana
appearing within a small dense central core. The cluster may contain an intermediate-mass black hole. The cluster was recorded in 1751-2 by Nicolas-Louis de
47_Tucanae
Dwarf spheroidal Galaxy in the constellation Leo
to the mass of the Milky Way's black hole, Sagittarius A*. However, another study could not confirm this, suggesting at most an intermediate-mass black
Leo_I_(dwarf_galaxy)
Masashi; et al. (25 June 2008). "Planetary Companions around Three Intermediate-Mass G and K Giants: 18 Delphini, ξ Aquilae, and HD 81688". Publications
List of proper names of exoplanets
List_of_proper_names_of_exoplanets
Hypothetical mechanism for extracting energy from rotating black holes
particle decay via the original (or classical) Penrose process is 20.7% of its mass in the case of an uncharged black hole (assuming the best case of maximal
Penrose_process
Supermassive black hole at the center of the Milky Way
2004, a team of astronomers reported the discovery of a potential intermediate-mass black hole, referred to as GCIRS 13E, orbiting 3 light-years from
Sagittarius_A*
Dwarf Galaxy in the constellation Ursa Major
ultraluminous X-ray source. One hypothesis suggests that is caused by an intermediate mass black hole that is pulling surrounding material. Holmberg II was discovered
Holmberg_II
Something that has mass and volume
Sohn, Sangmo Tony; Wyn Evans, N. (12 March 2019). "Evidence for an Intermediate-mass Milky Way from Gaia DR2 Halo Globular Cluster Motions". The Astrophysical
Matter
Layer of cells in mammalian embryos
The intermediate mesoderm or intermediate mesenchyme is a narrow section of the mesoderm (the middle germ layer) located between the paraxial mesoderm
Intermediate_mesoderm
Galaxy in the constellation Fornax
Chandra suggests that a white dwarf star has been torn apart by an intermediate-mass black hole, but this is only a proposal, and its true nature remains
NGC_1399
Astronomical objects
Vela X-1 4U 0352+309 Bursting Pulsar Vela Junior LMC N49 Intermediate-mass X-ray binary High-mass X-ray binaries Centaurus X-3 Circinus X-1 GX 301-2 Hercules
List_of_neutron_stars
Ballistic missile with a range of 3,000–5,500 km
An intermediate-range ballistic missile (IRBM) is a ballistic missile with a range between 3,000 and 5,500 kilometres (1,900–3,400 mi), categorized between
Intermediate-range ballistic missile
Intermediate-range_ballistic_missile
Division of elementary particles
62.1 GeV. The weakened bound opens up a neutrino decay channel for intermediate mass Higgs, and interesting multi-particle final states for Higgs and fourth
Generation_(particle_physics)
Gas giant exoplanet
(2026). "A transiting hot Jupiter with two outer siblings orbiting an intermediate-mass post main-sequence star". Monthly Notices of the Royal Astronomical
TOI-375_d
Globular cluster in the constellation Scorpius
that this extended horizontal branch may be the result of a central intermediate mass black hole (IMBH). X-ray observations of the cluster rule out an accreting
NGC_6388
Small spiral galaxy, containing one of the smallest central black holes
nucleus (AGN). It is centered on a lighter intermediate-mass black hole which is predicted to have a mass of 10^4.1 or ~12,500 M☉, making it one of the
UGC_8153
Galaxy in the constellation Coma Berenices
member of the Virgo Cluster. NGC 4298 may harbor an intermediate-mass black hole with an estimated mass ranging from 20,000 (2×104 M☉) to 500,000 (5×105
NGC_4298
Star in the constellation Crux
Gomes da Silva, J.; et al. (November 2023). "Planets around evolved intermediate-mass stars. III. Planet candidates and long-term activity signals in six
NGC_4349-127
Globular cluster in the constellation Hercules
needed] In 2007, a paper was published suggesting the possibility of an intermediate-mass black hole of up to 13,000 solar masses at the centre of the cluster
Messier_13
Star not gravitationally bound to any galaxy
matter problem. It was also suggested that the tidal destruction of intermediate-mass galaxies may have been a plausible contributor to the existence and
Intergalactic_star
INTERMEDIATE MASS
INTERMEDIATE MASS
Surname or Lastname
English
English : habitational name from a place in North Yorkshire called Masongill. The surname has died out in England.
Surname or Lastname
English
English : variant of Masongill (see Massengill).
Surname or Lastname
English
English : variant of Masongill (see Massengill).
Surname or Lastname
English
English : occupational name for a stonemason, Anglo-Norman French machun, a Norman dialect variant of Old French masson (see Mason).
Surname or Lastname
English (Midlands)
English (Midlands) : possibly a variant of Messer.
Surname or Lastname
English
English : variant of Masongill (see Massengill).
Girl/Female
Indian, Sanskrit
Intermediate Region
Male
English
Variant spelling of English Driscoll, DRISKOLL means "go-between, intermediary, messenger, news bearer."Â
Male
Italian
Italian form of Latin Maximilian, MASSIMILIANO means "the greatest."
Surname or Lastname
English and Scottish (of Norman origin) and French
English and Scottish (of Norman origin) and French : habitational name from any of various places in northern France which get their names from the Gallo-Roman personal name Maccius + the locative suffix -acum.English (of Norman origin) : habitational name from Marcy in La Manche. This surname is preserved in the English place name Stondon Massey.English : from a pet form of Matthew.Altered spelling of French Massé (see Masse 4).
Surname or Lastname
English
English : from a medieval personal name, a survival of Old English Mæssa, which came to be taken as a pet form of Matthew.English : possibly a metonymic occupational name for a mace-bearer, from Old French masse ‘mace’.English : habitational name from Macé in Orne, France.French (Macé) : variant of Massey; also a vernacular form of the personal name Mathieu (see Matthew).
Male
Italian
Italian form of Latin Maximus, MASSIMO means "the greatest."
Surname or Lastname
English
English : variant of Massey.
Surname or Lastname
English
English : variant of Massey.Ukrainian : from the personal name Matei (see Matthew).
Male
Hebrew
(מַשָׂ×) Hebrew name MASSA means "burden." In the bible, this is the name of a son of Ishmael.
Surname or Lastname
English
English : variant of Masongill (see Massengill).
Surname or Lastname
Dutch
Dutch : occupational name for a hawker or travelling salesman, Middle Dutch me(e)rseman.Dutch : habitational name for someone from any of numerous places named ter or de Meers(ch).German : unexplained; possibly a variant of Massmann.English : unexplained.
Surname or Lastname
English
English : variant of Mace 1.French (Picardy) : metonymic occupational name from masse ‘mace’, ‘hammer’.French : habitational name from places called Masse (Allier and Cô-d’Or), or La Masse (Eure, Lot, Puy-de-Dôme, Saône-et-Loire).French (Massé) : habitational name from a place called Massé in Maine-et-Loire, so named from Gallo-Roman Macciacum (from the personal name Maccius + the locative suffix -acum).Dutch : from Middle Dutch masse ‘clog’; ‘cudgel’, perhaps a metonymic occupational name for someone who wielded a club.Dutch : possibly a variant of Maas 1, or a patronymic from Mas.
Surname or Lastname
German
German : nickname for someone with boils or lumpy skin, or perhaps for a hunchback, from Middle High German maser ‘lump’, ‘protuberance’.German and English : from Middle High Germanmaser, Middle English maser ‘maple-wood bowl’ (Old French masere, of Germanic origin), hence a metonymic occupational name for a wood-turner producing such ware.English : variant spelling of Macer, an occupational name for a mace-bearer, from Old French maissier, massier, a derivative of Old French masse ‘mace’.German (Maaser) : pet form of Thomas.
Surname or Lastname
English and French
English and French : from the medieval personal name Masselin. This originated as an Old French pet form of Germanic names with the first element mathal ‘speech’, ‘counsel’. However, it was later used as a pet form of Matthew. Compare Mace. A feminine form, Mazelina, was probably originally a pet form of Matilda.English and French : possibly a metonymic occupational name for a maker of wooden bowls, from Middle English, Old French maselin ‘bowl or goblet of maple wood’ (a diminutive of Old French masere ‘maple wood’, of Germanic origin). In some cases it may derive from the homonymous dialect terms maslin, one of which means ‘brass’ (Old English mæslen, mæstling), the other ‘mixed grain’ (Old French mesteillon).
INTERMEDIATE MASS
INTERMEDIATE MASS
Boy/Male
British, English
Spring
Boy/Male
Muslim/Islamic
Brave
Boy/Male
Irish
Little raven.
Boy/Male
Hindu
Rational
Boy/Male
Indian
Combination of Durga and Ishwar
Boy/Male
Hindu, Indian, Marathi, Tamil
The Sun
Boy/Male
Native American
Sacred.
Girl/Female
French English Teutonic
Boy/Male
Tamil
Shamindra | ஷமிநà¯à®¤à¯à®°
Quiet, Gentle
Boy/Male
Bengali, Hindu, Indian, Marathi, Telugu, Traditional
Most Beloved Like Gems; Lord Hanuman
INTERMEDIATE MASS
INTERMEDIATE MASS
INTERMEDIATE MASS
INTERMEDIATE MASS
INTERMEDIATE MASS
a.
Lying between; intervening; intermediate.
a.
Lying or being in the middle place or degree, or between two extremes; coming or done between; intervening; interposed; interjacent; as, an intermediate space or time; intermediate colors.
a.
Intermediate.
n.
Intermediate time or space; interval.
a.
Intermediate.
a.
Lying, coming, or done, between; intermediate; as, an intermediary project.
n.
Intermediate agency.
n.
An intermediate agent.
n. pl.
The middle pair of tail feathers, or middle rectrices.
v. i.
To come between; to intervene; to interpose.
n.
Intermediate action.
n.
An intermediate or connecting link.
n.
A mediator.
n.
One who, or that which, is intermediate; an interagent; a go-between.
a.
Intermediate.
n.
Intermediate space.
n.
Interposition; intervention.
n.
Hence, intermediate argument or discussion.
a.
Intermediate; intervening.
adv.
In an intermediate manner; by way of intervention.