AI & ChatGPT searches , social queries for ULTRA DIFFUSE-GALAXY
Search references for ULTRA DIFFUSE-GALAXY. Phrases containing ULTRA DIFFUSE-GALAXY
See searches and references containing ULTRA DIFFUSE-GALAXY!
Search references for ULTRA DIFFUSE-GALAXY. Phrases containing ULTRA DIFFUSE-GALAXY
See searches and references containing ULTRA DIFFUSE-GALAXY!ULTRA DIFFUSE-GALAXY
Extremely low luminosity galaxy
An ultra diffuse galaxy (UDG), or dark galaxy, is an extremely low luminosity galaxy, the first example of which was discovered in the nearby Virgo Cluster
Ultra_diffuse_galaxy
Hypothesized galaxy with no, or very few, stars
astronomers reported that Dragonfly 44, an ultra diffuse galaxy (UDG) with the mass of the Milky Way galaxy, but with nearly no discernible stars or galactic
Dark_galaxy
Ultra diffuse galaxy in the constellation Cetus
NGC 1052-DF2 is an ultra diffuse galaxy (UDG) identified in a wide-field imaging survey of the NGC 1052 group by the Dragonfly Telephoto Array. It has
NGC_1052-DF2
Dark galaxy in the Perseus cluster
was indeed a galaxy. It is the first galaxy to be detected through the presence of globular clusters. Unlike most ultra-diffuse galaxies that have been
CDG-2
Galaxy in constellation Coma Berenices
Dragonfly 44 is an ultra diffuse galaxy in the Coma Cluster. This galaxy is well-known because observations of the velocity dispersion in 2016 suggested
Dragonfly_44
Ultra diffuse galaxy in the Perseus–Pisces Supercluster
DGSAT I is a quenched, ultra diffuse galaxy (UDG) located on the outskirts of the Pisces-Perseus Supercluster, identified in 2016 during a visual inspection
DGSAT_I
Low surface-brightness dwarf satellite galaxy of the Milky Way
brightness of any galaxy discovered and is ~ 100 times more diffuse than any known ultra diffuse galaxy. The large size of the galaxy suggests that it
Antlia_II
galaxy Ultra diffuse galaxy Field galaxy Galactic tide Galaxy cloud Interacting galaxy Galaxy merger Jellyfish galaxy Satellite galaxy Stellar kinematics
Outline_of_galaxies
System of stars and interstellar matter
of (dwarf) irregular galaxies include the Magellanic Clouds. A dark or "ultra diffuse" galaxy is an extremely-low-luminosity galaxy. It may be the same
Galaxy
Galaxy cluster in the constellation Virgo
Way. The elliptical galaxies are more centrally concentrated than the spiral galaxies. The first example of an ultra-diffuse galaxy was also found in the
Virgo_Cluster
Constellation straddling the celestial equator
elliptical galaxy NGC 1052 and the ultra-diffuse galaxy NGC 1052-DF2. IC 1613 (Caldwell 51) is an irregular dwarf galaxy near the star 26 Ceti and is a member
Cetus_(constellation)
Galaxy in the constellation Virgo
truncated—possibly by an encounter with another galaxy. Its interstellar medium consists of diffuse gas enriched by elements emitted from evolved stars
Messier_87
Galaxy which is less bright than the ambient night sky
A low-surface-brightness galaxy, or LSB galaxy, is a diffuse galaxy with a surface brightness that, when viewed from Earth, is at least one magnitude lower
Low_surface_brightness_galaxy
Galaxy in the constellation Virgo
(400,000 to 550,000 light-years). It possesses a diffuse core, which is the largest core of any galaxy known to date, and contains a supermassive black
IC_1101
Chemical enriched dwarf galaxy
higher than expected ratio of [Mg/Ca] than other metal poor stars in ultra-diffuse galaxies. The chemical enrichment of Grus ll is from the stellar nucleosynthesis
Grus_II
Australian astronomer known for work on galaxy structure and supermassive black holes
remnant nuclei of tidally stripped galaxies, and ultra-diffuse galaxies (UDGs) as an extension of brighter early-type galaxy structural scaling relations.
Alister_Graham
Galaxy in the constellation Pegasus
detection of 89 candidate ultra-diffuse galaxies (UDGs), around NGC 7609 and HCG 95, in which one is linked with. It is a gas-rich galaxy with H i mass 1.1 x
NGC_7609
Galaxy containing the Solar System
Way or Milky Way Galaxy, or simply the Galaxy, is the galaxy that includes the Solar System, with the name describing the galaxy's appearance from Earth:
Milky_Way
Spiral galaxy in the constellation Triangulum
Triangulum Galaxy's brightest and largest H II region (diffuse emission nebula containing ionized hydrogen) as H III.150 separately from the galaxy itself;
Triangulum_Galaxy
Topics referred to by the same term
Montenegro Uracil-DNA glycosylase (UDG), an enzyme Ultra diffuse galaxy (UDG), an extremely low luminosity galaxy UDG Healthcare, an Irish healthcare support
UDG
Intermediate spiral galaxy in the constellation Sculptor
The Sculptor Galaxy (also known as the Silver Coin Galaxy, Silver Dollar Galaxy, NGC 253, or Caldwell 65) is an intermediate spiral galaxy in the constellation
Sculptor_Galaxy
Cluster of galaxies in the constellation Coma Berenices
outskirts of the cluster. Some of the galaxies in the Coma Cluster have also been identified as ultra diffuse galaxies. The full extent of the cluster was
Coma_Cluster
Galaxy that orbits a larger galaxy due to gravitational attraction
of host galaxies, globular clusters should not be mistaken for satellite galaxies. Satellite galaxies are not only more extended and diffuse compared
Satellite_galaxy
trillion+ galaxies occupy the observable universe. On the order of 100,000 galaxies make up the Local Supercluster, and about 51 galaxies are in the
List_of_galaxies
Unsolved problem in physics
galaxies showed that massive dwarf galaxies tend to be more cuspy compared to lower-mass dwarf galaxies. More recently, a nearby ultra diffuse galaxy
Cuspy_halo_problem
2016 Android smartphones by Samsung Electronics
user break the screen on a Galaxy S7. On September 23, 2016, a make-up artist’s Samsung Galaxy S7 Edge started to diffuse smoke in a beauty salon in Antipolo
Samsung_Galaxy_S7
Hypothesis proposing a modification of Newton's laws
polarization enhance the gravitational attraction between baryons. Some ultra diffuse galaxies, such as NGC 1052-DF2, originally appeared to be free of dark matter
Modified_Newtonian_dynamics
Magellanic Clouds? Gaia Proper Motions of the Recently Discovered Ultra-faint Galaxies". The Astrophysical Journal. 867 (1): 19. arXiv:1805.01448. Bibcode:2018ApJ
List_of_nearest_galaxies
Galaxy in the constellation Leo
Leisman, Lukas; Fielder, Catherine E. (2023-01-01). "Gas-rich, Field Ultra-diffuse Galaxies Host Few Gobular Clusters". The Astrophysical Journal. 942 (1):
KKh_060
Galaxies bound to the Milky Way
(13 April 2016). "The feeble giant. Discovery of a large and diffuse Milky Way dwarf galaxy in the constellation of Crater". Monthly Notices of the Royal
Satellite galaxies of the Milky Way
Satellite_galaxies_of_the_Milky_Way
Galaxy in the constellation Virgo
example of an ultra diffuse galaxy. Ultra-diffuse galaxies have higher proportions of globular clusters than other galaxies, but NGC 5846 is one of the
NGC_5846
– Astronomers report that Dragonfly 44, an ultra diffuse galaxy (UDG) with the mass of the Milky Way galaxy, but with nearly no discernable stars or galactic
2016_in_science
Galaxies with interacting gravitational fields
Interacting galaxies, also known as colliding galaxies, are two or more galaxies whose gravitational fields result in a disturbance of one another. There
Interacting_galaxy
Pressure due to movement through a fluid medium
K.; Romanowsky, A. J. (May 2017). "The HI content of isolated ultra-diffuse galaxies: A sign of multiple formation mechanisms?". Astronomy & Astrophysics
Ram_pressure
Type-cD elliptical galaxy in the constellation of Ursa Major
radio galaxy with a 1.4 GHz luminosity range between 2 × 1023 and 3 × 1025 W Hz−1. It has an ellipsoidal stellar halo measuring ~80 kpc with two diffuse ultra-steep
2MASX_J10222849+5006200
Multiple exposure image of deep space in the constellation Ursa Major
Hubble Ultra-Deep Field. The HDF galaxies contained a considerably larger proportion of disturbed and irregular galaxies than the local universe; galaxy collisions
Hubble_Deep_Field
Unsolved problem in cosmology
place: Finding dwarf galaxies is an extremely difficult task, since they tend to have low surface brightness and are highly diffuse – so much so that they
Dwarf_galaxy_problem
Matter and radiation in the space between the star systems in a galaxy
background star field of the galaxy; the most prominent are listed in his Barnard Catalogue. The first direct detection of cold diffuse matter in interstellar
Interstellar_medium
Type of starburst galaxy
medium conditions at z ~ 5.5–9.5 with ultra-deep JWST/NIRSpec spectroscopy" (diagram top right) examines 27 galaxies at high redshifts that were observed
Blueberry_galaxy
Curved path of an object around a point
Carleton, Timothy; et al. (2021). "An excess of globular clusters in Ultra-Diffuse Galaxies formed through tidal heating". Monthly Notices of the Royal Astronomical
Orbit
Natural physical entity in space
ice and dust, and an object in reference to the entire comet with its diffuse coma and tail. According to NASA astrophysicists, early astronomical objects
Astronomical_object
Hypothetical invisible cosmic material
matter forms planets, stars, and galaxies. Observations so far suggest dark matter doesn't do that – it resides only in diffuse halos ... As a result, it is
Dark_matter
Plasma that cosmologists believe exists between galaxies
current epoch. The WHIM can be described as a web of hot, diffuse plasma stretching between galaxies, as well as atoms and molecules, in contrast to dark matter
Warm–hot_intergalactic_medium
Constellation in the northern hemisphere
supermassive black hole in its center. M91 (NGC 4548), a barred spiral galaxy with a bright, diffuse nucleus, is the faintest object in Messier's catalog at magnitude
Coma_Berenices
History and future of the universe
attraction also gradually pulls galaxies towards each other to form groups, clusters and superclusters. Hubble Ultra Deep Field observations has identified
Chronology_of_the_universe
Globular cluster
discrete X-ray sources Terzan 5 produces a diffuse non-thermal X-ray emission and high (a few GeV) and ultra-high (0.5–24 TeV) energy gamma-rays. The high
Terzan_5
Astrophysical phenomenon
completely destroyed to form a diffuse nebula. The peak optical luminosity of a supernova can be comparable to that of an entire galaxy before fading over several
Supernova
Theoretical upper limit on the energy of cosmic ray protons
the limit. These theories propose that ultra-high energy cosmic rays are produced nearby the Milky Way galaxy or that Lorentz covariance is violated in
Greisen–Zatsepin–Kuzmin_limit
Constellation in the southern celestial hemisphere
Dwarf galaxy is a small faint satellite galaxy of the Milky Way. NGC 1316 is a relatively close radio galaxy. The Hubble Space Telescope's Ultra-Deep Field
Fornax
Type of cosmic ray
System from beyond the Milky Way galaxy. While at low energies, the majority of cosmic rays originate within the Galaxy (such as from supernova remnants)
Extragalactic_cosmic_ray
Void between celestial bodies
exists beyond Earth's atmosphere and between celestial bodies. It contains ultra-low levels of particle densities, constituting a near-perfect vacuum of
Outer_space
Galaxy in the constellation Hydra
metal-rich and metal-poor clusters. A large population of about 50 ultra-compact dwarf galaxies (UDCs) have been detected in the Hydra Cluster, with most of
NGC_3311
Large, low-density interstellar cloud of partially ionized gas
composition of galaxies. Spiral and irregular galaxies contain many H II regions, while elliptical galaxies are almost devoid of them. In spiral galaxies, including
H_II_region
Physical phenomenon from outside of the Earth's atmosphere
the Sun or other regions of the sky, such as the center of the Milky Way Galaxy. Celestial objects like quasars, which are super dense objects far from
Cosmic_noise
Low-surface brightness Milky Way satellite dwarf galaxy in the constellation Eridanus
cluster. The stability of this cluster, near the center of such a small, diffuse, galaxy places constraints on the nature of dark matter (Brandt 2016; Li et
Eridanus_II
Two colliding clusters of galaxies in constellation Carina
retrieved December 27, 2016 Milgrom, Mordehai (2015-12-21). "Ultra-diffuse cluster galaxies as key to the MOND cluster conundrum" (PDF). Monthly Notices
Bullet_Cluster
Galaxy in the constellation of Boötes
up diffused radio emission is seen extending by 35 kiloparsecs between the galaxies. The nucleus on the eastern side of the double nucleus galaxy in the
IRAS_14394+5332
1990s astrophysics experiment in Utah
The Chicago Air Shower Array (CASA) was a significant ultra high high-energy astrophysics experiment operating in the 1990s. It consisted of a very large
Chicago_Air_Shower_Array
Absorption features in astronomical spectra
Diffuse interstellar bands (DIBs) are absorption features seen in the spectra of astronomical objects in the Milky Way and other galaxies. They are caused
Diffuse_interstellar_bands
Galaxy filament
The Coma Filament is a galaxy filament. The filament contains the Coma Supercluster of galaxies and forms a part of the CfA2 Great Wall. Abell catalogue
Coma_Filament
Edge-on spiral galaxy in the constellation Virgo
5170 is 3.4×1012 M☉. Examination of the galaxy with the Chandra X-ray Observatory showed there is no diffuse X-ray emission from hot gas in the extended
NGC_5170
Possible type of luminous blue compact galaxy
May 2021). "An Old Stellar Population or Diffuse Nebular Continuum Emission Discovered in Green Pea Galaxies". The Astrophysical Journal Letters. 912
Pea_galaxy
Measurement of electromagnetic radiation for astronomy
from the Earth. As of January 2013, the largest galaxy redshift of z~12 was found using the Hubble Ultra-Deep Field, corresponding to an age of over 13
Astronomical_spectroscopy
Astrophysical maser, source of stimulated spectral line emission
hundred billion solar luminosities, or LFIR > 1011 L☉, and ultra-luminous infrared galaxies (ULIRGs), with LFIR > 1012 L☉ are favored. These infrared luminosities
Megamaser
Galaxy filament containing the Perseus-Pisces Supercluster
The Perseus–Pegasus Filament is a galaxy filament containing the Perseus–Pisces Supercluster and stretching for over a billion light-years (or over 300/h
Perseus–Pegasus_Filament
European undersea neutrino detector
neutrino oscillations, atmospheric muons, diffuse neutrino flux, point-like source emission, Starburst Galaxies, core collapse supernova, and combined analyses
KM3NeT
Galaxy in the constellation Hercules
nucleus of the galaxy is active and it has been classified as a radio galaxy with an ultra steep radio spectrum. When observed, it has two extended radio lobes
IC_1262
Galaxy filament
Ursa Major Filament is a galaxy filament. The filament is connected to the CfA Homunculus, a portion of the filament forms a portion of the "leg" of the
Ursa_Major_Filament
Galaxy filament
Lynx–Ursa Major Filament (LUM Filament) is a galaxy filament. The filament is connected to and separate from the Lynx–Ursa Major Supercluster. Abell, G
Lynx–Ursa_Major_Filament
Radio galaxy located in the constellation Boötes
with an ultra-steep spectrum, it is likely the radio emission is contaminating the galaxy. A tail extension has been discovered in the galaxy making the
UGC_8669
Astronomical object emitting X-rays
X-rays. Several types of astrophysical objects emit X-rays. They include galaxy clusters, black holes in active galactic nuclei (AGN), galactic objects
Astrophysical_X-ray_source
Theoretical device to render objects invisible
combined with the properties of the metamaterial coating. When light is diffused, a thin coat of metamaterial around an object can make it essentially invisible
Cloaking_device
center of Abell 133, there is an active galaxy that is hosting an Active Galactic Nuclei (AGN) and a large, diffuse filamentary cloud of radio emission or
Abell_133
Cosmological process in the early universe
Ebeling, Harald; Egami, Eiichi; Clement, Benjamin (2015-11-18). "Are ultra-faint galaxies at z = 6–8 responsible for cosmic reionization? Combined constraints
Reionization
Observational astronomy performed with gamma rays
of galaxies, including the Crab Nebula and the Vela Pulsar (the most powerful source so far), have been identified, alongside an overall diffuse gamma-ray
Gamma-ray_astronomy
10 parsecs, or 32.6 light-years. accretion disk A roughly circular mass of diffuse material in orbit around a central object, such as a star or black hole
Glossary_of_astronomy
Isotope of hydrogen with one neutron
Milky Way galaxy than expected, or perhaps deuterium has been replenished by a large in-fall of primordial hydrogen from outside the galaxy. In space
Deuterium
Elementary particle with extremely low mass
Way (our own galaxy). In addition to the detection of neutrinos from individual supernovae, it should also be possible to detect the diffuse supernova neutrino
Neutrino
Musical artist
Records, Diffused Records, and Juicy Music, among others. In late 2014, he released his track "Generic," which had earlier debuted at the Ultra Festival
Makj
star-forming structures form from the diffuse interstellar medium? How do these structures interact with the ISM? Galaxy rotation problem: Is dark matter (solely)
List of unsolved problems in astronomy
List_of_unsolved_problems_in_astronomy
Division of astronomy
measure other phenomena in that neighborhood, including the distance to a galaxy. Galileo Galilei turned a telescope to the heavens and recorded what he
Observational_astronomy
Observation of infrared wavelengths
that intergalactic dust greatly dims the light of distant galaxies. In actuality, galaxies are almost twice as bright as they look. The dust absorbs much
Infrared_astronomy
Fictional universe created by Iain M. Banks
advanced technology relative to most other civilisations it shares the galaxy with. Most of the Culture's citizens do not live on planets but in artificial
The_Culture
Diode that emits light from an organic compound
proper application of a circular polarizer and antireflective coatings, the diffuse reflectance can be reduced to less than 0.1%. With 10,000 fc incident illumination
OLED
Penetrating form of electromagnetic radiation
ray photons have photon energy at the lower end from 104 eV to 107 eV; ultra-high-energy gamma rays have energies over 1014 eV. Paul Villard, a French
Gamma_ray
Citizen science project
Radio Galaxy Zoo (RGZ) is an internet crowdsourced citizen science project that seeks to locate supermassive black holes in distant galaxies. It is hosted
Radio_Galaxy_Zoo
high redshift galaxies performed with the Infrared Space Observatory (ISO) ELF – extremely luminous far-infrared galaxy, a synonym for Ultra-Luminous infrared
List_of_astronomy_acronyms
Telescope carried by a balloon
Transient Antenna, an ultra-high-energy cosmic neutrinos detector ARCADE 2006–2011 Absolute Radiometer for Cosmology, Astrophysics, and Diffuse Emission, a NASA
Balloon-borne_telescope
McLintock, G. A.; Thomas, R. E. (December 1972). "Modelling of the double-diffused MOST's with self-aligned gates". 1972 International Electron Devices Meeting
List of semiconductor scale examples
List_of_semiconductor_scale_examples
by looking at the 21-cm line emission produced by hot diffuse neutral hydrogen from distant galaxy clusters and from the intracluster medium. This neutral
Hydrogen Intensity and Real-time Analysis eXperiment
Hydrogen_Intensity_and_Real-time_Analysis_eXperiment
High-energy particle, mainly originating outside the Solar System
narrow band of gamma ray intensity produced in discrete and diffuse sources in our galaxy, and numerous point-like extra-galactic sources distributed
Cosmic_ray
X-ray optics design that mimics the structure of lobster eyes
(Sheath Transport Observer for the Redistribution of Mass/Diffuse X-ray emission from the Local galaxy) had micropore reflectors arranged in an array to form
Lobster-eye_optics
Observing low-mass stellar particles
large, meaning that photons produced in the core will take a long time to diffuse outward. Therefore, neutrinos are the only way that we can obtain real-time
Neutrino_astronomy
Inverse relationship between the intensity and duration
Researches – Part V. On the Measurement of the Chemical Action of Direct and Diffuse Sunlight". Proceedings of the Royal Society. 12: 306–312. Bibcode:1862RSPS
Reciprocity_(photography)
Star at the centre of the Solar System
of the heat outward to the Sun's photosphere above. Once the material diffusively and radiatively cools just beneath the photospheric surface, its density
Sun
why do these appear at different frequency ratios in different objects? Diffuse interstellar bands: What is responsible for the numerous interstellar absorption
List of unsolved problems in physics
List_of_unsolved_problems_in_physics
Hypothetical travel between stars or planetary systems
Bussard ramjet, a fusion rocket in which a huge scoop would collect the diffuse hydrogen in interstellar space, "burn" it on the fly using a proton–proton
Interstellar_travel
1996 film directed by Jonathan Frakes
lights near the ceiling and took advantage of a large window to shine diffused lights through. To give the scene a black-and-white feel, Leonetti made
Star_Trek:_First_Contact
ultra-relativistic gas near a very massive black hole at the galaxy's center. Lastly, a diffuse X-ray emission was found to exist all over the sky. The study
History_of_X-ray_astronomy
Retrieved 2025-10-06. Robinson, Joe (2012-09-28). "Best Hidden Tracks". Diffuser.fm. Retrieved 2025-10-12. Pareles, Jon (June 5, 2005). "The Case Against
List of albums containing a hidden track
List_of_albums_containing_a_hidden_track
ULTRA DIFFUSE-GALAXY
ULTRA DIFFUSE-GALAXY
ULTRA DIFFUSE-GALAXY
ULTRA DIFFUSE-GALAXY
ULTRA DIFFUSE-GALAXY
ULTRA DIFFUSE-GALAXY
ULTRA DIFFUSE-GALAXY
ULTRA DIFFUSE-GALAXY
ULTRA DIFFUSE-GALAXY