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Satellite galaxy of the Milky Way
The Large Magellanic Cloud (LMC) is a dwarf galaxy and satellite galaxy of the Milky Way. At a distance of around 50 kiloparsecs (163,000 light-years)
Large_Magellanic_Cloud
Two dwarf galaxies orbiting the Milky Way
as Magellanic spiral galaxies. The two galaxies are the following: Large Magellanic Cloud (LMC), about 163 kly (50 kpc) away Small Magellanic Cloud (SMC)
Magellanic_Clouds
Dwarf irregular galaxy, satellite galaxy of the Milky Way
The Small Magellanic Cloud (SMC) is a dwarf galaxy near the Milky Way. Classified as a dwarf irregular galaxy, the SMC has a D25 isophotal diameter of
Small_Magellanic_Cloud
Spiral galaxies with one spiral arm
SBm, SABm); the prototype galaxy and namesake for Magellanic spirals is the Large Magellanic Cloud, an SBm galaxy. They are usually smaller dwarf galaxies
Magellanic_spiral
SAGE-Spec Spitzer Legacy program: the life-cycle of dust and gas in the Large Magellanic Cloud. Point source classification – III". Monthly Notices of the Royal
List_of_largest_stars
Heterogeneous class of stars with unusual spectra
somewhat lower in M31, lower still in the Large Magellanic Cloud, and much lower in the Small Magellanic Cloud. Strong metallicity variations are seen across
Wolf–Rayet_star
HVCld in Sculptor by MClds
The Magellanic Stream is a stream of high-velocity clouds of gas extending behind the Large and Small Magellanic Clouds over 100° through the Galactic
Magellanic_Stream
H II region in the constellation Dorado
The Tarantula Nebula (also known as 30 Doradus) is a large H II region in the Large Magellanic Cloud (LMC), forming its south-east corner (from Earth's
Tarantula_Nebula
cluster in Large Magellanic Cloud. BSDL 2527 is a star cluster in Large Magellanic Cloud. DEM S10 is a H II region in Small Magellanic Cloud. DEM S80 is
List_of_most_massive_stars
Wolf–Rayet star in the constellation Dorado
bright stars in the Large Magellanic Cloud (LMC). Among the objects cataloged was RMC 136 (Radcliffe observatory Magellanic Cloud catalog number 136)
R136a1
List from the Alphabet Direction (αβ)
— The Fourth Catalogue of Population I Wolf Rayet stars in the Large Magellanic Cloud BAY — Uranometria (Bayer designation) BCVS — Bibliographic Catalogue
List of astronomical catalogues
List_of_astronomical_catalogues
of the Large Magellanic Cloud. This is a list of luminous blue variable stars in order of their distance from Earth. The Large Magellanic Cloud (LMC) is
List of luminous blue variable stars
List_of_luminous_blue_variable_stars
Star in the constellation Dorado
BAT99-98 is a Wolf–Rayet star located in the Large Magellanic Cloud, in NGC 2070 near the R136 cluster in the Tarantula Nebula (30 Doradus). At estimates
BAT99-98
H II region in the Large Magellanic Cloud
(N70) is a faint emission nebula and superbubble located in the Large Magellanic Cloud in the constellation of Dorado. Henize 70 was first observed in
Henize_70
Super star cluster in the constellation Dorado, in the Large Magellanic Cloud
cluster, which lies at the centre of the Tarantula Nebula in the Large Magellanic Cloud. When originally named it was an unresolved stellar object (catalogued
R136
Large, low-density interstellar cloud of partially ionized gas
thousands of stars. Examples include the 30 Doradus region in the Large Magellanic Cloud and NGC 604 in the Triangulum Galaxy. The term H II is pronounced
H_II_region
Binary star in the constellation Dorado
WOH G64 (IRAS 04553–6825) is a symbiotic binary in the Large Magellanic Cloud, roughly 50 kiloparsecs (163,000 light-years) from Earth. The primary component
WOH_G64
Group of galaxies that includes the Milky Way
satellite system comprises the Sagittarius Dwarf Galaxy, Large Magellanic Cloud, Small Magellanic Cloud, Canis Major Dwarf Galaxy (disputed, considered by some
Local_Group
Red supergiant star in the constellation Dorado
referred to as [W60] B90) is a large and highly luminous red supergiant star similar to Betelgeuse in the Large Magellanic Cloud. It is one of the largest
B90_(star)
Small galaxy composed of up to several billion stars
stars, as compared to the Milky Way's 100–400 billion stars. The Large Magellanic Cloud, which closely orbits the Milky Way and contains over 30 billion
Dwarf_galaxy
Stars sorted by absolute magnitude
Large Magellanic Cloud. DEM S10 is a H II region in Small Magellanic Cloud. FSR 1555 is a star cluster. DEM S80 is a H II region in Small Magellanic Cloud
List_of_most_luminous_stars
Extraterrestrial view of outer space
would be easily visible to the naked eye. From a viewpoint in the Large Magellanic Cloud, the Milky Way's total apparent magnitude would be −2.0—over 14
Extraterrestrial_sky
2008. "Magellanic Cloud". Astronomy Knowledge Base. University of Ottawa. Archived from the original on 5 July 2006. "The Large Magellanic Cloud, LMC"
List_of_galaxies
Constellation in the southern sky
also been depicted as a swordfish. Dorado contains most of the Large Magellanic Cloud, the remainder being in the constellation Mensa. The South Ecliptic
Dorado
Galaxy morphological classification scheme advocated by Edwin Hubble
fork. Examples of irregular galaxies: M82, NGC 1427A, Large Magellanic Cloud, Small Magellanic Cloud. Elliptical and lenticular galaxies are commonly referred
Hubble_sequence
Astrophysical phenomenon
observed was Kepler's Supernova in 1604. SN 1987A occurred in the Large Magellanic Cloud, a satellite galaxy of our galaxy, in 1987. Several thousand supernovae
Supernova
Interstellar absorption and scattering of light
extinction curves are those of the Milky Way, the Small Magellanic Cloud (SMC) and the Large Magellanic Cloud (LMC). In the LMC, there is significant variation
Extinction_(astronomy)
American astronomer (1889–1953)
Gravitational Lensing Experiment. Cepheids in the Magellanic Clouds. IV. Catalog of Cepheids from the Large Magellanic Cloud". Acta Astronomica. 49: 223–317. arXiv:astro-ph/9908317
Edwin_Hubble
Cavity hundreds of light years across created by strong stellar winds in a galaxy
Perseus-Taurus Shell The Local Bubble Very Large Telescope image of superbubble LHA 120-N 44 in the Large Magellanic Cloud. Credit: ESO/Manu Mejias. The Per-Tau
Superbubble
Type of star that is luminous, blue, and variable in brightness
Doradus variables after S Doradus, one of the brightest stars of the Large Magellanic Cloud. The LBV stars P Cygni and η Carinae have been known as unusual
Luminous_blue_variable
Emission nebula in the constellation Dorado
is an emission nebula with superbubble structure located in the Large Magellanic Cloud, a satellite galaxy of the Milky Way in the constellation Dorado
N44_(emission_nebula)
Spiral galaxy in the constellation Triangulum
second-smallest spiral galaxy in the Local Group after the Large Magellanic Cloud, which is a Magellanic-type spiral galaxy. It is believed to be a satellite
Triangulum_Galaxy
System for categorizing galaxies based on appearance
“Magellanic” spirals and irregulars, respectively, after the Magellanic Clouds. The Large Magellanic Cloud is of type SBm, while the Small Magellanic Cloud
Galaxy morphological classification
Galaxy_morphological_classification
Large self-illuminated object in space
pressure on the accreting gas cloud. Several stars in the R136 cluster in the Large Magellanic Cloud have been measured with larger masses, but it has been
Star
Star cluster in the constellation Dorado
NGC 1910, or LH-41, is an OB association in the Large Magellanic Cloud. NGC 1910's right ascension is 5h 18m 42.5s and its declination is -69° 14′ 12.1″
NGC_1910
X-ray binaries in Large Magellanic Cloud
LMC X-3 is a high-mass X-ray binary (HMXB) system located in the Large Magellanic Cloud (LMC), a satellite galaxy of the Milky Way approximately 165,000
LMC_X-3
Hypergiant star in the constellation Dorado
HD 32034 (or R 62) is one of seven blue hypergiants in the Large Magellanic Cloud and is suspected to be a shell star. It lies within the loose association
HD_32034
System of stars and interstellar matter
to the unaided eye, including the Andromeda Galaxy, Large Magellanic Cloud, Small Magellanic Cloud, and the Triangulum Galaxy. In the 10th century, Persian
Galaxy
Open cluster in the constellation Dorado
cluster located in the Dorado constellation and is part of the Large Magellanic Cloud. It is not visible to the naked eye and requires a telescope to
NGC_2003
Globular cluster in the Large Magellanic Cloud
located within the Large Magellanic Cloud in the constellation Dorado. Compared to other globular clusters of the Large Magellanic Cloud, NGC 2005 has a
NGC_2005
original on 2019-05-17. Retrieved 2019-05-17. "N70 Nebula in the Large Magellanic Cloud". www.eso.org. Archived from the original on 15 November 2018. Retrieved
List_of_largest_nebulae
Type of variable star that pulsates radially
Henrietta Swan Leavitt after studying thousands of variable stars in the Magellanic Clouds. The discovery establishes the true luminosity of a Cepheid by observing
Cepheid_variable
Physics apparatus designed to study neutrinos
2018[update] are the Sun and the supernova 1987A in the nearby Large Magellanic Cloud. Another likely source (three standard deviations) is the blazar
Neutrino_detector
1998 American film
(Peter Boyle) claims that they originated in the Large Magellanic Cloud (also called the Magellanic Galaxy), due to it apparently being the only other
Species_II
Galaxy that orbits a larger galaxy due to gravitational attraction
is the Large Magellanic Cloud. Moreover, satellite galaxies are not the only astronomical objects that are gravitationally bound to larger host galaxies
Satellite_galaxy
Supernova visible from Earth in the 17th century
galaxy have been seen since S Andromedae in 1885. SN 1987A in the Large Magellanic Cloud was visible to the naked eye at night. Evidence exists for two Milky
Kepler's_Supernova
Stream of neutral hydrogen gas linking the two Magellanic clouds
stream of stars throughout the Magellanic Bridge linking the Large Magellanic Cloud (LMC) with the Small Magellanic Cloud (SMC). This stellar bridge is
Magellanic_Bridge
Star in the Large Magellanic Cloud
Doradus (also known as S Dor) is one of the brightest stars in the Large Magellanic Cloud (LMC), a satellite galaxy of the Milky Way, located roughly 160
S_Doradus
Star in the constellation Dorado
hypergiant in the Large Magellanic Cloud. It is surrounded by an unexpected dust disk. R126, formally RMC (Radcliffe observatory Magellanic Cloud) 126, is a
HD_37974
1973 science fiction novel by Arthur C. Clarke
to propel itself out of the Solar System in the direction of the Large Magellanic Cloud. After Rama leaves, a member of the Rama Committee considers that
Rendezvous_with_Rama
Rare star with tremendous luminosity and high rates of mass loss by stellar winds
general characteristics of LBV spectral lines. S Doradus, in the Large Magellanic Cloud, in the southern constellation of Dorado. Prototype variable, LBVs
Hypergiant
Spiral shaped H II region in the constellation Dorado
LHA 120-N 119) is a spiral-shaped H II region in the Large Magellanic Cloud. Its dimensions are large, at 131 x 175 pc (430 × 570 ly). It contains several
N119
Supernova remnant in the constellation Mensa
(also known as SNR 0509–68.7) is a supernova remnant located in the Large Magellanic Cloud. It is relatively close to Earth, allowing astronomers to observe
N103B
Wolf Rayet star in the constellation Dorado
VFTS 682 is a Wolf–Rayet star in the Large Magellanic Cloud. It is located over 29 parsecs (95 ly) north-east of the massive cluster R136 in the Tarantula
VFTS_682
Galaxy morphological types and objects that are members of the Large Magellanic Cloud are identified using the NASA/IPAC Extragalactic Database. The other
List of NGC objects (1001–2000)
List_of_NGC_objects_(1001–2000)
1987 supernova event in the constellation Dorado
SN 1987A was a Type II supernova in the Large Magellanic Cloud, a dwarf satellite galaxy of the Milky Way. It occurred approximately 51.4 kiloparsecs (168
SN_1987A
Star in Large Magellanic Cloud
HD 37836 is a candidate luminous blue variable located in the Large Magellanic Cloud and one of the brightest stars in its galaxy. The star was first mentioned
HD_37836
Emission nebula in the constellation Dorado
is the brightest emission nebula in the north-west part of the Large Magellanic Cloud in the Dorado constellation. The N11 complex is the second largest
N11_(emission_nebula)
Red emission nebula in the constellation Dorado
red emission nebula surrounding an open cluster of stars in the Large Magellanic Cloud, at a distance of about 163,000 light-years. The nebula was discovered
NGC_2014
Nebula in the Large Magellanic Cloud
LMC N79 (or LHα 120-N79) is an emission nebula in the Large Magellanic Cloud. The nebula is part of the catalog of H-alpha stars and nebulae by Karl G
LMC_N79
Class of galaxy
irregular galaxies. The Large Magellanic Cloud has since been re-classified as type SBm (barred Magellanic spiral). The Small Magellanic Cloud remains classified
Irregular_galaxy
Open star cluster within the Large Magellanic cloud
cluster located in the Dorado constellation which is part of the Large Magellanic Cloud. It was discovered by John Herschel on November 30, 1834. Its apparent
NGC_1997
Star in the constellation Dorado
concentration of stars of the large NGC 2070 open cluster in the Tarantula Nebula, a massive H II region in the Large Magellanic Cloud which is a nearby satellite
R136a2
O-type main sequence star in the constellation Dorado
BI 253 is an O2V star in the Large Magellanic Cloud and is a primary standard of the O2 type. It is one of the hottest main-sequence stars known and one
BI_253
Subclass of pulsating star
standard candles. They have been used to establish the distance to the Large Magellanic Cloud, globular clusters, open clusters, and the Galactic Center. The
Delta_Scuti_variable
Globular star cluster
NGC 2210 is a globular cluster located in the Large Magellanic Cloud, in the constellation Dorado. It is situated south of the celestial equator and, as
NGC_2210
Spherical collection of stars
clusters contain multiple populations; the globular clusters in the Large Magellanic Cloud (LMC) exhibit a bimodal population, for example. During their youth
Globular_cluster
Open cluster in the constellation Dorado
cluster located in the Dorado constellation and is part of the Large Magellanic Cloud. NGC 2001 was discovered by James Dunlop on September 27, 1826.
NGC_2001
Star in the Large Magellanic Cloud
R71 (RMC 71, HD 269006) is a star in the Large Magellanic Cloud (LMC) in the constellation Mensa. It is classified as a luminous blue variable and is one
R71_(star)
Open cluster in the constellation Dorado
2710, LH 9) is an open cluster in the Dorado constellation in the Large Magellanic Cloud. It encompasses a group of about 50 massive hot young stars. These
NGC_1761
Study of the movement of stars
velocities, or even ejected. A large-scale example is the gravitational interaction between the Milky Way and the Large Magellanic Cloud. A supernova explosion
Stellar_kinematics
Emission nebula in the constellation Dorado
surrounding the Wolf-Rayet star BAT99-59. It is located in the Large Magellanic Cloud. The nebula was discovered on 30 December 1836 by polymath John
NGC_2020
Supernova in the constellation Dorado
supergiant star, located on the outskirts of the Tarantula Nebula in the Large Magellanic Cloud. It was the progenitor of supernova 1987A. The star was originally
Sanduleak_−69_202
Wolf–Rayet star in the constellation Dorado
LMC195-1 is a Wolf–Rayet star located in the Large Magellanic Cloud (LMC). It is an extremely rare member of the WO oxygen sequence, at WO2 the hottest
LMC195-1
Emission nebula in the constellation Dorado
as N 180B (LHA 120-N 180B), is an emission nebula located in the Large Magellanic Cloud. "Hubble heritage project". Results for N 180B. Archived from the
NGC_2122
Large Magellanic Cloud nebula in the constellation Mensa
Henize 206 is a nebula in the Large Magellanic Cloud. This luminous cloud of gas and dust houses a cluster of newborn stars. Although Henize 206 was first
Henize_206
Type of neutron star with a strong magnetic field
that had exploded as a supernova around 3000 BCE. It was in the Large Magellanic Cloud and the event was named GRB 790305b, the first-observed SGR megaflare
Magnetar
Remnants of an exploded star
young supernova remnants was formed by SN 1987A, a supernova in the Large Magellanic Cloud observed in February 1987. Other well-known supernova remnants include
Supernova_remnant
Star cluster in the Dorado constellation
having an aperture of 6 inches (150mm) or more. It is located in the Large Magellanic Cloud and is estimated to be between 45 and 50 light years across. Tadross
NGC_2009
Open cluster in the constellation Dorado
NGC 1860 is an open cluster in the Large Magellanic Cloud in the constellation Dorado. It was discovered in 1836 by John Herschel with an 18.7-inch reflecting
NGC_1860
Star in the constellation Dorado
repeater (SGR), located in the supernova remnant LMC N49, in the Large Magellanic Cloud. It was the first soft gamma repeater discovered, and as of 2015
SGR_0526−66
Irregular version of a barred spiral galaxy
shape. Examples include the Large Magellanic Cloud (LMC) and NGC 6822, although LMC is more often classified as a magellanic spiral galaxy. Some barred
Barred_irregular_galaxy
Topics referred to by the same term
navigation Magellanic Clouds, two major Milky Way neighbouring galaxies, matter streams, or systems related to them: Large Magellanic Cloud, a major satellite
Magellanic
Star in the constellation Mensa
Space Telescope in the Milky Way's nearest neighbor galaxy, the Large Magellanic Cloud (the other being R 126 or HD 37974), as being circled by monstrous
HD_268835
Star in the Large Magellanic cloud
R99 (HD 269445) is a star in the Large Magellanic Cloud in the constellation Dorado. It is classified as a possible luminous blue variable and is one of
R99_(star)
Contact binary star system in the constellation Dorado
light years away in the Tarantula Nebula, which is part of the Large Magellanic Cloud. It is the most massive and earliest spectral type overcontact system
VFTS_352
Yellow hypergiant in the Large Magellanic Cloud
an Alpha Cygni variable. It is one of the brightest stars in the Large Magellanic Cloud (LMC), positioned in the deep southern constellation of Dorado.
HD_271182
Sakurai [ja]. Sanduleak's Star is a possible symbiotic star in the Large Magellanic Cloud (LMC). Named after Nicholas Sanduleak. The Sanduleak–Pesch Binary
Stars_named_after_people
2009 video game
2010. The science fiction storyline, set across the Small and Large Magellanic Clouds, follows the life and growth of Yuri as he first confronts the
Infinite_Space
Gravitational process studied in astronomy
Star formation is the process by which dense regions within molecular clouds in interstellar space—sometimes referred to as "stellar nurseries" or "star-forming
Star_formation
Astronomical phenomenon due to the gravitational lens effect
bulge. The first two microlensing events in the direction of the Large Magellanic Cloud that might be caused by dark matter were reported in back to back
Gravitational_microlensing
Binary star in the Large Magellanic cloud
30 Doradus complex (also known as the Tarantula Nebula) in the Large Magellanic Cloud. Both components are amongst the most massive and most luminous
Melnick_34
Nebula in the constellation Dorado
N41, LHA 120-N 41) is an emission nebula in the north part of the Large Magellanic Cloud in the Dorado constellation. Originally catalogued in Karl Henize's
N41_(nebula)
Massive star in the Large Magellanic Cloud
O-type star located in the Tarantula Nebula (30 Doradus) within the Large Magellanic Cloud (LMC). Identified as part of the VLT-FLAMES Tarantula Survey (VFTS)
VFTS_16
Star in the constellation Dorado
spectroscopic binary star system in the LH 54 OB association within the Large Magellanic Cloud in the constellation Dorado. The OB association LH 54 was catalogued
LH_54-425
Star cluster in the constellation Dorado
NGC 1852 is a star cluster in the Large Magellanic Cloud in the constellation Dorado. It was discovered in 1826 by James Dunlop with a 9-inch reflecting
NGC_1852
Star in the constellation Dorado
LMC X-1 is the first X-ray source detected in the Large Magellanic Cloud. It was discovered in 1969, using data from an instrument carried by a Sandia
LMC_X-1
Massive blue supergiant star in the constellation Dorado
is a massive blue supergiant star in the Tarantula Nebula in the Large Magellanic Cloud located in the constellation Dorado. Although it is only 21 times
Melnick_42
Constellation in the southern celestial hemisphere
Alpha Mensae, is barely visible in suburban skies. Part of the Large Magellanic Cloud, several star clusters and a quasar lie in the area covered by the
Mensa_(constellation)
aliens. The Cotati originated on Hala in the Pama star system in the Large Magellanic Cloud, the same planet as the warlike humanoid Kree race. The Dire Wraiths
List of alien races in Marvel Comics
List_of_alien_races_in_Marvel_Comics
LARGE MAGELLANIC-CLOUD
LARGE MAGELLANIC-CLOUD
Girl/Female
English
Lark.
Boy/Male
American, Australian, Chinese, Irish, Welsh
Large Homestead; Great Settlement; Large Village
Surname or Lastname
English
English : variant of Sark.German : unexplained.
Girl/Female
American, Australian
Combination of Latonia and Ray
Surname or Lastname
English and French
English and French : nickname (literal or ironic) meaning ‘generous’, from Middle English, Old French large ‘generous’, ‘free’ (Latin largus ‘abundant’). The English word came to acquire its modern sense only gradually during the Middle Ages; it is used to mean ‘ample in quantity’ in the 13th century, and the sense ‘broad’ first occurs in the 14th. This use is probably too late for the surname to have originated as a nickname for a fat man.
Surname or Lastname
English (mainly Norfolk)
English (mainly Norfolk) : variant of Lark 1.
Girl/Female
American, Australian, British, English
Skylark; Lark
Boy/Male
Australian, Welsh
Large Homestead; Large Settlement
Boy/Male
Dutch
Large.
Surname or Lastname
English and French
English and French : metonymic occupational name for a boatman, from Middle English, Old French barge ‘boat’, ‘barge’.Dutch : variant of Berg.
Boy/Male
American, Australian, British, Celtic, Christian, English, French, German, Irish, Jamaican, Welsh
Prudent; Large Homestead; Large Settlement
Boy/Male
French
The red-haired one.
Girl/Female
Persian American
Child of light. Famous Bearer: Margaret Thatcher, former Prime Minister of the United Kingdom.
Boy/Male
Hindu, Indian
Large
Girl/Female
Swedish
From the sea.
Boy/Male
Tamil
Large quantity
Female
English
Short form of English Margaret, MARGE means "pearl."
Girl/Female
British, English
Intelligent
Boy/Male
Dutch Anglo Saxon
Tall.
Boy/Male
British, English
Large
LARGE MAGELLANIC-CLOUD
LARGE MAGELLANIC-CLOUD
Girl/Female
Hindu
Gentle, Creator
Boy/Male
Indian
Agent, Representative
Biblical
establishing, or revenging, of Jehovah,whom Jehovah gathers
Girl/Female
Indian
Goddess Lakshmi
Girl/Female
Arabic, Australian, Indian, Muslim
Form; Figure; Complexion
Girl/Female
Tamil
Anumitha | அநà¯à®‚மீதா
Love and kindness
Boy/Male
Hindu, Indian, Sanskrit
Full of Mercy; Kind
Boy/Male
Arabic, Bengali, Gujarati, Hindu, Indian, Kannada, Malayalam, Marathi, Muslim, Telugu
Talented
Boy/Male
Hindu, Indian
Protector
Girl/Female
Hindu, Indian, Marathi, Tamil
Beauty Redefined
LARGE MAGELLANIC-CLOUD
LARGE MAGELLANIC-CLOUD
LARGE MAGELLANIC-CLOUD
LARGE MAGELLANIC-CLOUD
LARGE MAGELLANIC-CLOUD
a.
Of or pertaining to, or named from, Magellan, the navigator.
n.
Specifically, the Magellanic clouds.
n.
A large, roomy boat for the conveyance of passengers or goods; as, a ship's barge; a charcoal barge.
adv.
Freely; licentiously.
a.
Having large hands, Fig.: Taking, or giving, in large quantities; rapacious or bountiful.
n.
A whirlwind, or whirlwind squall, encountered in the Straits of Magellan.
superl.
Abundant; ample; as, a large supply of provisions.
n.
A movement or piece in largo time.
superl.
Having more than usual power or capacity; having broad sympathies and generous impulses; comprehensive; -- said of the mind and heart.
superl.
Full in statement; diffuse; full; profuse.
n.
A musical note, formerly in use, equal to two longs, four breves, or eight semibreves.
n.
A large boat used by flag officers.
a.
Having a large or generous heart or disposition; noble; liberal.
superl.
Unrestrained by decorum; -- said of language.
superl.
Exceeding most other things of like kind in bulk, capacity, quantity, superficial dimensions, or number of constituent units; big; great; capacious; extensive; -- opposed to small; as, a large horse; a large house or room; a large lake or pool; a large jug or spoon; a large vineyard; a large army; a large city.
a.
Made large or larger; extended; swollen.
superl.
Crossing the line of a ship's course in a favorable direction; -- said of the wind when it is abeam, or between the beam and the quarter.
n.
A large omnibus used for excursions.
superl.
Prodigal in expending; lavish.
superl.
Free; unembarrassed.