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Cloud of heated and ionized gas and dust in the constellation Cygnus
as Caldwell 33), whose brightest area is NGC 6992, trailing off farther south into NGC 6995 (together with NGC 6992 also known as "Network Nebula") and
Veil_Nebula
This is a list of NGC objects 3001–4000 from the New General Catalogue (NGC). The astronomical catalogue is composed mainly of star clusters, nebulae
List of NGC objects (3001–4000)
List_of_NGC_objects_(3001–4000)
Reflection nebula in the constellation Cepheus
The Iris Nebula (also known as NGC 7023 or Caldwell 4) is a bright reflection nebula located about 1,300 light years from Earth in the constellation of
Iris_Nebula
Lenticular galaxy in the constellation Virgo
seen by William Herschel in 1784 with his 47 cm (19 in) telescope. NGC 4452 is so thin that it is actually difficult to determine what type of disk galaxy
NGC_4452
Galaxy in constellation Canes Venatici
dimensions, means that NGC 4111 is about 55,000 light-years across. It was discovered by William Herschel in 1788. NGC 4111 possesses both thin and thick discs
NGC_4111
Satellite galaxy of the Andromeda Galaxy
Antonaldo (1 November 2016). "The potential role of NGC 205 in generating Andromeda's vast thin corotating plane of satellite galaxies". Monthly Notices
Messier_110
Galaxy in the constellation Canes Venatici
Messier 106 (also known as NGC 4258) is an intermediate spiral galaxy in the constellation Canes Venatici. It was discovered by Pierre Méchain in 1781
Messier_106
Galaxy in the constellation Perseus
density (less than 2 M⊙/pc). NGC 1167 has ring-like arcs where star formation is taking place. However its arcs are uncommonly thin and smooth, not showing
NGC_1167
Spiral galaxy in the constellation Leo
Catalogue. NGC 3604 has a small bright nucleus with inner spiral arms. There is evidense of star formation near the centre. There are thin smooth spiral
NGC_3604
Galaxy in the constellation Vela
NGC 3256 is a peculiar galaxy formed from the collision of two separate galaxies in the constellation of Vela. NGC 3256 is located about 122 million light-years
NGC_3256
Spiral galaxy in the constellation Draco
2009). "Aperture Synthesis Observations of the Nearby Spiral NGC 6503: Modeling the Thin and Thick H I Disks". The Astronomical Journal. 137 (6): 4718–4733
NGC_6503
Galaxy in the constellation Virgo
NGC 4496 is a pair of galaxies in the constellation of Virgo. Individually, the larger, northern galaxy is designated NGC 4496A, and the smaller, southern
NGC_4496
Planetary nebula in the constellation Camelopardalis
NGC 1501 is a planetary nebula with a complex structure, located in the northern constellation of Camelopardalis. It has the proper names Camel's Eye
NGC_1501
Globular cluster in the constellation Musca
Doodad Nebula (Sandqvist 149), a 3° thin streak of black across a southern section of the great plane of the Milky Way. NGC 4372 "is partially obscured by
NGC_4372
Galaxy in the constellation Crater
NGC 3513 is a barred spiral galaxy in the constellation Crater. The galaxy lies about 40 million light years away from Earth, which means, given its apparent
NGC_3513
Galaxy in the constellation of Virgo
NGC 5506 is a spiral galaxy located in the constellation Virgo. It is located at a distance of about 75 million light years from Earth, which, given its
NGC_5506
Planetary nebula in Lyra
stars Beta and Gamma Lyrae. It is also catalogued as Messier 57, M57 and NGC 6720. The nebula was discovered by Charles Messier in 1779. It has an apparent
Ring_Nebula
Galaxy in the constellation Dorado
NGC 1596 is a lenticular galaxy in the constellation Dorado. The galaxy lies about 55 million light years away from Earth, which means, given its apparent
NGC_1596
Galaxy in the constellation Leo
stellar velocity dispertion in the pseudobulge of NGC 3338 is 78 ± 2 km/s. The galaxy has two thin and well ordered spiral arms, but its overall pattern
NGC_3338
Galaxy in the constellation Puppis
colleagues described NGC 2566 as a: Nuclear point source embedded in a large slightly elliptical bulge. Bulge is threaded by a long, thin, bright bar. Underlying
NGC_2566
Galaxy in the constellation Lepus
December 1786. The galaxy features two thin arcs which contain HII regions. The galaxy forms a pair with NGC 1957 [fr], which lies 5.1 arcminutes away
NGC_1954
Remains of a galaxy merger in the Milky Way
members are Messier 2, Messier 56, Messier 75, Messier 79, NGC 1851, NGC 2298, and NGC 5286. NGC 2808 is another globular-like cluster of the Sausage. It
Gaia_Sausage
Galaxy in the constellation Virgo
the interacting pair Arp 271 (NGC 5426 and NGC 5427), NGC 5476, and NGC 5493. Six supernovae have been observed in NGC 5468: SN 1999cp (Type Ia, mag.
NGC_5468
Open cluster in the constellation Gemini
old thin disk population. It was first classed as such by Trumpler but later Shapley would classify it as an open cluster due to its diffuse core. NGC 2158
NGC_2158
Galaxy in the constellation Crater
NGC 3887 is a barred spiral galaxy in the constellation Crater. The galaxy lies about 55 million light years away from Earth, which means, given its apparent
NGC_3887
Contraction of an astronomical object due to the influence of its gravity
NGC 6745 produces material densities sufficiently extreme to trigger star formation through gravitational collapse
Gravitational_collapse
Constellation in the southern celestial hemisphere
being long and thin (16' by 3'). In the eyepiece of a large telescope, its southeastern dust lane becomes visible. Another galaxy is NGC 5102, found by
Centaurus
Spiral galaxy in the constellation Ursa Major
suggested, it hasn't been proven. The galaxy has multiple well-defined thin arms. NGC 4096 is asymmetric in the north–south axis, with the northern half having
NGC_4096
It is a member of the young thin disk population of the Milky Way. In 2021, D. Camargo presented results that suggested NGC 1605 is actually a binary open
NGC_1605
Galaxy in the constellation Draco
Spectrograph reported the presence of a thin disk of material around a supermassive black hole at the center of NGC 3147. The black hole is 250 million times
NGC_3147
Edge-on spiral galaxy in the constellation Virgo
with NGC 5170. Numerical modeling of this galaxy indicates it has a massive dark halo with a thin, low surface brightness disk. The halo mass of NGC 5170
NGC_5170
Galaxy that orbits a larger galaxy due to gravitational attraction
Dwarf elliptical satellite galaxies in the Local Group include NGC 147, NGC 185, and NGC 205, which are satellites of our neighboring Andromeda galaxy
Satellite_galaxy
System of stars and interstellar matter
right/bottom): NGC 7541, NGC 3021, NGC 5643, NGC 3254, NGC 3147, NGC 105, NGC 2608, NGC 3583, NGC 3147, MRK 1337, NGC 5861, NGC 2525, NGC 1015, UGC 9391, NGC 691
Galaxy
Open cluster in the constellation Cassiopeia
NGC 189 is an open cluster in the Cassiopeia constellation. It was discovered by Caroline Herschel on 27 September 1783, and independently rediscovered
NGC_189
Type of sealed coin holder
original on 23 July 2023. Retrieved 23 July 2023. "Evolution of the NGC Holder". NGC Coin. Numismatic Guaranty Company. Archived from the original on 9
Coin_slab
Galaxy in the constellation Serpens
arms the Milky Way galaxy has. The central bar is very small, long and thin. NGC 5964 thus does not have a galactic habitable zone like the Milky Way.
NGC_5964
Disputed galaxy located near the constellation Canis Major
Globular clusters thought to be associated with the CMa include NGC 1851, NGC 1904, NGC 2298 and NGC 2808, all of which may have been part of the galaxy's globular
Canis_Major_Overdensity
Historical local supercluster home to the Milky Way
extension), Leo II, Virgo III, Crater (NGC 3672), Leo I, Leo Minor (NGC 2841), Draco (NGC 5907), Antlia (NGC 2997), and NGC 5643. Of the luminous galaxies located
Virgo_Supercluster
Galaxy in the constellation of Piscis Austrinus
NGC 7172 is a spiral galaxy located in the constellation Piscis Austrinus. It is located at a distance of about 110 million light years from Earth, which
NGC_7172
Galaxy in the constellation Fornax
means that NGC 1381 is about 55,000 light years across. It is a member of the Fornax Cluster. NGC 1381 appears edge-on and features a thin disk with high
NGC_1381
Spiral galaxy in the constellation Virgo
NGC 5775 is a spiral galaxy, a member of the Virgo Cluster, that lies at a distance of about 70 million light-years. Although the spiral is tilted away
NGC_5775
Spiral galaxy in the constellation Leo
(2023). "The vertical structure of the spiral galaxy NGC 3501: First stages of the formation of a thin metal-rich disc". Monthly Notices of the Royal Astronomical
NGC_3501
Galaxy in the constellation Leo Minor
NGC 3504 is a barred spiral galaxy in the constellation Leo Minor. It has a Hubble distance corresponding to 88 million light-years and was discovered
NGC_3504
Interacting galaxy pair in the constellation of Ursa Major
NGC 4194, the Medusa merger, is a galaxy merger in the constellation Ursa Major about 128 million light-years (39.1 Mpc) away. It was discovered on April
NGC_4194
Spiral galaxy in the constellation Virgo
NGC 4939 is a large spiral galaxy located in the constellation Virgo. It is located at a distance of about 120 million light years from Earth, which,
NGC_4939
Lenticular galaxy in the constellation Andromeda
galaxies that forms the group are NGC 79, NGC 81, NGC 83, NGC 85, NGC 86, Arp 65 (NGC 90 and NGC 93, NGC 94, NGC 96, IC 1542 and IC 1546. According to astronomers
NGC_80
Galaxy in the constellation Virgo
Messier 87 (also known as Virgo A or NGC 4486, generally abbreviated to M87) is a supergiant elliptical galaxy in the constellation Virgo that contains
Messier_87
Type of star that is luminous, blue, and variable in brightness
290 (Romano's star, an unusually hot LBV) NGC 2403: V12 V37 V38 J025941.21+251412.2 J025941.54+251421.8 NGC 2363-V1 J122809.72+440514.8 J122817.83+440630
Luminous_blue_variable
Lines radiating from bright light sources in photographs
cluster Westerlund 1 with diffraction spikes JWST image of the spiral galaxy NGC 7469 with diffraction spikes Iris diaphragms with moving blades are used
Diffraction_spike
Retrieved 28 October 2022. "The Topsy-Turvy Galaxy NGC 1313". ESO. 23 November 2006. "NGC 2683". NGC Online. SEDS. Retrieved 4 February 2014. Karen Masters
List_of_galaxies
Barred spiral galaxy in the Local Group
originally named the Andromeda Nebula and is cataloged as Messier 31, M31, and NGC 224. Andromeda has a D25 isophotal diameter of about 46.56 kiloparsecs (152
Andromeda_Galaxy
Galaxy in the constellation Hercules
NGC 6264 is an active Seyfert galaxy located in the constellation of Hercules. The redshift of the galaxy is (z) 0.033 and it was first discovered in
NGC_6264
which have shown evidence of extraplanar gas include NGC 891, NGC 2403, UGC 7321, NGC 4559 and NGC 3198. Possible explanations for the presence of this
Extraplanar_gas
Spiral galaxy in the constellation Cetus
middle". NGC 681 shares many structural similarities with the Sombrero Galaxy, M104, although it is smaller, less luminous, and less massive. Its thin, dusty
NGC_681
Type of emission nebula created by dying red giants
In 1782, William Herschel, discoverer of Uranus, found the Saturn Nebula (NGC 7009) and described it as "A curious nebula, or what else to call it I do
Planetary_nebula
Constellation in the northern celestial hemisphere
star. Within the constellation's borders lie NGC 2419, an unusually remote globular cluster; the galaxy NGC 2770, which has hosted three recent Type Ib
Lynx_(constellation)
Galaxies with interacting gravitational fields
formation, and AGN activity are closely intertwined in shaping galaxy evolution. NGC 7318 "HubbleSite: News - Hubble Finds that "Blue Blobs" in Space Are Orphaned
Interacting_galaxy
Planetary nebula in the constellation Scorpius
double-shell structure. NGC 6153 has a Peimbert type of I, indicating it is helium and nitrogen rich and the progenitor was a thin disk star. A 1986 analysis
NGC_6153
Compact astronomical body
Very Long Baseline Array observed H 2O masers as they orbited the centre of NGC 4258, a galaxy with a similar central mass. The orbital parameters ruled
Black_hole
Spiral or lenticular galaxy in the constellation Cygnus
structure except for a faint, thin spiral-like feature running through the galaxy. The neutral atomic hydrogen distribution in NGC 7013 is mostly located in
NGC_7013
Galaxy in the constellation Hydra
categorised as a type II Seyfert galaxy. Even though NGC 3081 shows significant absorption, it is Compton thin[clarification needed]. Also it does not show spectral
NGC_3081
Constellation in the southern celestial hemisphere
stars are only a few million years old. Lying 2 degrees southwest of NGC 2362 is NGC 2354 a fainter open cluster of magnitude 6.5, with around 15 member
Canis_Major
Galaxy in the constellation Coma Berenices
barred lenticular. The star formation rate is 0.11±0.02 M☉·yr−1. NGC 4710 possesses both thin and thick discs. Gonzalez, Oscar A.; et al. (March 2017). "Peanut-shaped
NGC_4710
Galaxy in the constellation Andromeda
by 4,700 globular clusters. Discovered in 1979 by Kotanyi et al., NGC 708 has a thin dust lane with an irregular structure. Besides the dust lane, there
NGC_708
Large, low-density interstellar cloud of partially ionized gas
distances in the universe, and the study of extragalactic H II regions (Such as NGC 604 and 206) is important in determining the distances and chemical composition
H_II_region
Galaxy in the constellation Columba
NGC 2188 is observed nearly edge-on from Earth, with its central bulge and spiral arms tilted away from the line of sight. As a result, only the thin
NGC_2188
Compact region at a galaxy's center with abnormally high luminosity
lines. Galaxies observed as part of this study included NGC 1068, NGC 4151, NGC 3516, and NGC 7469. Active galaxies such as these are known as Seyfert
Active_galactic_nucleus
Galaxy in the constellation Pisces
NGC 7679 is a lenticular galaxy with a peculiar morphology in the constellation Pisces. It is located at a distance of about 200 million light years from
NGC_7679
Structure formed by diffuse material in orbital motion around a massive central body
thin disks. The classic 1974 work by Shakura and Sunyaev on thin accretion disks is one of the most often quoted papers in modern astrophysics. Thin disks
Accretion_disk
Galaxy in the constellation Andromeda
magnitude is 13.7. NGC 90 is a grand-design spiral galaxy with two tidal arms extending from the main grand design arms. They are thin and long with one
NGC_90
U.S. currency
struck with the same (higher) pressure used for the steel cents. In 2019, NGC authenticated a worn 1943 cent composed of 86.41% tin and 8.37% antimony
1943_steel_cent
Galactic X-ray source in the constellation Cygnus that is very likely a black hole
relatively modest explosion). The compact object is thought to be orbited by a thin, flat disk of accreting matter known as an accretion disk. This disk is intensely
Cygnus_X-1
Current denomination of United States currency
Archived 2009-08-02 at the Wayback Machine. USA Today. Retrieved July 12, 2006. NGC History of the Roosevelt Dime. Archived 2011-07-14 at the Wayback Machine
Dime_(United_States_coin)
Gravitational effect also known as the differential force and the perturbing force
Figure 1: Tidal interaction between the spiral galaxy NGC 169 and a smaller companion
Tidal_force
Tightly packed group of stars within a larger formation
higher rate (per area) than is typically found in outer disks, as shown in NGC 4314 (see photo). Properties such as spiral structure and young stars suggest
Galactic_bulge
Constellation in the northern celestial hemisphere
a faint nebula, is accompanied by the bright open cluster NGC 1893. The cluster is thin, with a diameter of 12 arcminutes and a population of approximately
Auriga
Class of galaxy that has spiral structures extending from their cores
extend from the center of barred and unbarred spiral galaxies. These long, thin regions resemble a spiral and thus give spiral galaxies their name. Naturally
Spiral_galaxy
Hypothetical type of dark matter in physics
Galaxies in the NGC 3109 association are moving away too rapidly to be consistent with expectations in the ΛCDM model. In this framework, NGC 3109 is too
Cold_dark_matter
Material world and its phenomena
The Earth's atmosphere is a key factor in sustaining the ecosystem. The thin layer of gases that envelops the Earth is held in place by gravity. Air is
Nature
Binary star system in the southern constellation Tucana
classification of F6 V. It is around 2.6 billion years old and a member of the thin disk population. The primary has about 1.66 times the mass of the Sun while
Rho_Tucanae
Red giant star in the constellation Cygnus
Messier 29 Messier 39 NGC 6811 NGC 6819 NGC 6834 NGC 6866 NGC 6871 NGC 6910 NGC 7011 NGC 7024 NGC 7031 NGC 7037 NGC 7044 NGC 7050 NGC 7093 Molecular clouds
Kepler-56
1991 video game
Archived from the original on November 8, 2016. Retrieved January 6, 2017. "NGC Magazine UK". Game Rankings. CBS Interactive. February 1, 2006. Archived
Final_Fantasy_IV
Dwarf planet in the Kuiper belt
atmospheric pressure and 1 million times less than Pluto's. Such an extremely thin atmosphere was not detected in observations of Makemake's 2011 stellar occultation
Makemake
Binary star in the constellation Norma
as responsible for the emission from the region of NGC 6164/65. In 1959, K. G. Heinze catalogued NGC 6164/65 as a planetary nebula and placed HD 148937
HD_148937
History and future of the universe
defects) remaining from the time before inflation were now distributed very thinly across the universe. It is not known exactly when the inflationary epoch
Chronology_of_the_universe
1998 high-speed train crash near Eschede, Germany
Root-Cause-Analysis.info. Archived from the original on 26 April 2023. 090120 NGC Seconds from the catastrophe[full citation needed] Modern Railways. December
Eschede_train_disaster
means "south"), specifically refers to the South Africa. Ngca – (pronounced "Ngc-ah", dental click) an expression of appreciation or admiration, similar to
List of South African slang words
List_of_South_African_slang_words
NASA/ESA/CSA space telescope launched in 2021
2022 Cosmic Cliffs of Carina Nebula (NGC 3324) (NIRCam) Carina Nebula (NGC 3324) (MIRI) Southern Ring Nebula (NGC 3132; Left: NIRCam; Right: MIRI) Webb's
James_Webb_Space_Telescope
Constellation in the northern celestial hemisphere
similar to those of recurring novae. M57, also known as the "Ring Nebula" and NGC 6720, at a distance of 2,550 light-years from Earth is one of the best known
Lyra
Examples include HD 114762 b (>11.68 MJ), Pi Mensae b (>10.312 MJ), and NGC 2423-3 b (>10.6 MJ). A complete list of more than 3,000 ultracool dwarfs
List_of_brown_dwarfs
Spiral galaxy in the constellation of Lynx
Observations of Superthin Galaxies. II. IC 2233 and the Blue Compact Dwarf NGC 2537". The Astronomical Journal. 135 (1): 291–318. arXiv:0709.4249. Bibcode:2008AJ
IC_2233
Pair of galaxies and interacting galaxies in the constellation Aries
the galaxies started diminishing. Mice Galaxies – two interacting galaxies NGC 4302 – an edge-on spiral galaxy Antennae Galaxies – two interacting galaxies
UGC_2369
among the densest known objects in the universe. New General Catalogue (NGC) night sky The appearance of the Earth's sky at nighttime, when the Sun is
Glossary_of_astronomy
neutron stars and black holes. The pair are located in the globular cluster NGC 1851. Two insect-like robots, a mini-bug and a water strider, are reported
2024_in_science
Chemical compound
from interstellar grains in the Becklin–Neugebauer Object and probably in NGC 2264-IR as well. This detection helped explain the physical shape of previously
Ammonia
Large self-illuminated object in space
hydrogen in the core; stars just above this limit have been located in the NGC 6397 cluster. The faintest red dwarfs in the cluster are absolute magnitude
Star
Proposed element found in astronomical observation of a nebula
hypothetical nebulium. As Henry Norris Russell put it, "Nebulium has vanished into thin air." Nebulae are typically extremely rarefied, much less dense than the
Nebulium
Earliest historical form of English language
art in heaven, 2 Sīe þīn nama ġehālgod. [ˈsiːy̯ ðiːn ˈnɒ.mɑ jeˈhɑːɫ.ɣod] Be thine name hallowed. Hallowed be thy name. 3 Tōbecume þīn rīċe, [ˌtoː.beˈku.me
Old_English
Pair of telescopes mounted side-by-side
magnifications. Some open clusters, such as the bright double cluster (NGC 869 and NGC 884) in the constellation Perseus, and globular clusters, such as M13
Binoculars
Binary star system in the constellation Pisces
Earth, it is located roughly 350 light-years distant from the Sun in the thin disk population of the Milky Way. The two components are designated Eta Piscium
Eta_Piscium
NGC THIN
NGC THIN
Surname or Lastname
English (mostly East Anglia)
English (mostly East Anglia) : unexplained.Vietnamese (Ông) : unexplained.Chinese : variant of Wang 1.Indonesian : unexplained.Filipino : unexplained.
Male
Vietnamese
Vietnamese name CÔNG means "skillful; industrious."
Surname or Lastname
English
English : probably a variant of Axsom. This name is concentrated in NC.
Boy/Male
English
Lord.
Boy/Male
Australian, British, Christian, Danish, English, French, German, Greek, Romanian, Swedish
Lord; People of Victory; Victorious Person; Diminutive of Dominick
Female
Vietnamese
Vietnamese name NGOC means "precious gem."
Surname or Lastname
English
English : probably a variant of Marshburn.Edward Mashburn came from London to Onslow Co., NC, in 1698.
Surname or Lastname
English (County Durham)
English (County Durham) : variant of Harts. In the U.S. this name is concentrated in NC.
Surname or Lastname
English
English : perhaps a patronymic (meaning ‘son of the butler’) from Burl.Aaron Burleson emigrated from England to NC in 1726.
Surname or Lastname
English
English : unexplained. In the U.S., this is a predominantly a southern name, with large concentrations in NC, SC, and GA.
Surname or Lastname
English
English : probably a variant of London. This is a predominantly southern name in the U.S., found mainly in NC, SC, GA, and TX.
Female
Chinese
beauty-august.
Male
Vietnamese
Vietnamese name THINH means "prosperous."
Surname or Lastname
English
English : variant of Eddings. This is a common name in TX, NC, and FL.
Surname or Lastname
English
English : unexplained. Perhaps a variant of Newborn. This name occurs frequently in NC.
Female
Vietnamese
Vietnamese name NGOC BICH means "precious jade."
Surname or Lastname
English
English : patronymic meaning ‘son of Robert’, common in central England (see Dobb).Arthur Dobbs (1689–1765) was born at Castle Dobbs, Co. Antrim, Ireland. In 1745 he purchased 400,000 acres of land in NC and was selected as governor in 1754. He married twice and his second wife, wed when he was age 73, was a girl in her teens from NC.
Male
Vietnamese
Vietnamese name HÙNG means "heroic."
Surname or Lastname
German and Dutch
German and Dutch : nickname from Middle High German nac, nacke, Middle Dutch necke ‘neck’, perhaps denoting someone with a stiff neck, in either the literal or figurative sense.English : from the Old Norse personal name Hnaki.
Male
Thai/Siamese
Thai name THINNAKORN means "sun."
NGC THIN
NGC THIN
Boy/Male
American, British, English
From the Powerful Mill
Boy/Male
Tamil
Sai Chandra | ஸாஇ சஂதà¯à®°
Sai baba
Girl/Female
Hindu
Red, Pleasant, Beautiful
Boy/Male
Hindu, Indian
One who Always have Power
Girl/Female
Hindu, Indian, Malayalam, Marathi
Smart; Pretty; Funny; Saintly
Boy/Male
French, German, Greek, Latin
Cheerful; Happy; Joyful; Variant of Hilary
Boy/Male
Biblical
Who proclaims God.
Boy/Male
Muslim
Kind, Bountiful, Graceful
Boy/Male
American, British, English
Wealthy Ruler
Boy/Male
French, Hawaiian, Hebrew, Hindu, Indian, Traditional
Corn or Grain
NGC THIN
NGC THIN
NGC THIN
NGC THIN
NGC THIN
n.
The act of thinking; mode of thinking; imagination; cogitation; judgment.
v. t.
To form an opinion by reasoning; to judge; to conclude; to believe; as, I think it will rain to-morrow.
a.
Somewhat thin.
a.
Having the faculty of thought; cogitative; capable of a regular train of ideas; as, man is a thinking being.
v. t.
To prick; to st?ng.
n.
Clothes; furniture; appurtenances; luggage; as, to pack or store one's things.
a.
In a thin manner; in a loose, scattered manner; scantily; not thickly; as, ground thinly planted with trees; a country thinly inhabited.
p. pr. & vb. n.
of Thin
v. i.
To grow or become thin; -- used with some adverbs, as out, away, etc.; as, geological strata thin out, i. e., gradually diminish in thickness until they disappear.
a.
Having a thin skin; hence, sensitive; irritable.
a.
Full of spirit of life; effervesc/ng, as liquors; sparkling; as, brick cider.
v. t.
To call anything to mind; to remember; as, I would have sent the books, but I did not think of it.
v. t.
To make thin (in any of the senses of the adjective).
n.
One who thinks; especially and chiefly, one who thinks in a particular manner; as, a close thinker; a deep thinker; a coherent thinker.
n.
One who thins, or makes thinner.
imp. & p. p.
of Thin
superl.
Slight; small; slender; flimsy; wanting substance or depth or force; superficial; inadequate; not sufficient for a covering; as, a thin disguise.
p. pr. & vb. n.
of Think
adv.
Not thickly or closely; in a seattered state; as, seed sown thin.
n.
The quality or state of being thin (in any of the senses of the word).