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Star cluster in the Draco constellation
LAMOST 1 is a star cluster in the constellation Draco. It has been disrupted and consists of a comoving star-stream with about 25,000 stars. The stars
LAMOST_1
Schmidt telescope in China
The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST), also known as the Guo Shoujing Telescope (Chinese: 郭守敬望远镜) after the 13th-century
LAMOST
Star in the constellation of Draco
observations using the Navy Precision Optical Interferometer. The secondary star is 1.8 magnitudes (at 700 nm) fainter than the primary star and was detected at
Thuban
Galaxy in the constellation Draco
Kepler-90e f g h i Kepler-296b c d e f TOI-1452 b TrES-2b Star clusters LAMOST 1 Nebulae Cat's Eye Nebula NGC 6742 Galaxies NGC 3147 3197 3735 3961 4121
3C_319
Dwarf Galaxy in the constellation Draco
Kepler-90e f g h i Kepler-296b c d e f TOI-1452 b TrES-2b Star clusters LAMOST 1 Nebulae Cat's Eye Nebula NGC 6742 Galaxies NGC 3147 3197 3735 3961 4121
PGC_39058
Overview of elongated streams of stars
Yong (23 December 2015). "LAMOST 1: A disrupted satellite in the constellation Draco". The Astrophysical Journal. 816 (1): L2 (5 pp). arXiv:1512.05090
List_of_stellar_streams
Galaxy in the constellation Draco
Seyfert 1 galaxy which is an X-ray source. "NASA/IPAC Extragalactic Database". Results for 3C 390.3. Retrieved 2006-10-26. "3CR 390.3 – Seyfert 1 Galaxy"
3C_390.3
Binary star system in the constellation Gemini
astronomers using the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) and the radial-velocity method to search for such wobbly stars. The astronomers
LB-1
Spectroscopic Telescope LAMOST" (PDF). Archived from the original (PDF) on July 22, 2011. the effective aperture in diameter is 3.6m - 4.9m "LAMOST Homepage – Gallery"
List of largest optical reflecting telescopes
List_of_largest_optical_reflecting_telescopes
Tidal disruption event in the constellation Draco
monitoring at radio and X-ray wavelengths indicated that after roughly 600 days (1.5 years), the relativistic jet shut off. This time likely corresponds with
Swift_J1644+57
Galaxy supercluster in the constellation Draco
Draco. It is located at a distance of 300 Mpc h−1 on a side of a void of diameter of about 130 Mpc h−1. The near side of the void is bordered by the Ursa
Draco_Supercluster
Star in the constellation Draco
irregular variable with a periodicity of roughly 1,100 days. It has an estimated 1.53 times the mass of the Sun and a measured radius of 70 times the radius
Lambda_Draconis
Radio galaxy in the constellation Draco
radio galaxies". Monthly Notices of the Royal Astronomical Society. 317 (1): 120–140. Bibcode:2000MNRAS.317..120R. doi:10.1046/j.1365-8711.2000.03684
3C_401
X-ray binary in the Whirlpool Galaxy
M51-ULS-1, also known as RX J132943+47115, is a high-mass X-ray binary (HMXB) system in the constellation of Canes Venatici. The binary system is located
M51-ULS-1
Active galaxy in the constellation Draco
dating back to 1895, and they suggest that this objects magnitude can vary by ±1.5. "3C 371". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved
3C_371
Quasar in the constellation Draco
an underestimate with log ( Δ M B H / M ⊙ ) ≥ 1 {\displaystyle \log(\Delta M_{BH}/M_{\odot })\geq 1} . Kolman et al. (1991) and Shapovalova (2016) independently
H1821+643
Star in the constellation Draco
proper names for stars. The WGSN approved the name Alruba for this star on 1 June 2018 and it is now so entered on the List of IAU-approved Star Names
Alruba
Star in the constellation Draco
shows under-abundances of carbon and oxygen in its spectrum. The star has 1.25 times the mass of the Sun and is an estimated 6.48 billion years old. It
Tau_Draconis
Galaxy cluster in the constellation Draco
Kepler-90e f g h i Kepler-296b c d e f TOI-1452 b TrES-2b Star clusters LAMOST 1 Nebulae Cat's Eye Nebula NGC 6742 Galaxies NGC 3147 3197 3735 3961 4121
CL1358+62
Star in the constellation Draco
velocities", Contributi Osservatorio Astronomico di Padova in Asiago, 239 (1): 1, Bibcode:1970CoAsi.239....1B. "rho Dra". SIMBAD. Centre de données astronomiques
Rho_Draconis
Binary star system in the constellation Draco
is 1.69±0.02 mas. At the estimated distance of Upsilon Draconis, this yields a physical size of about 19 times the Sun's radius. It is about 1.37 billion
Upsilon_Draconis
Star in the constellation Draco
oldest known star atlas". Journal of Astronomical History and Heritage. 12 (1): 39–59. arXiv:0906.3034. Bibcode:2009JAHH...12...39B. doi:10.3724/SP.J.1440-2807
7_Draconis
Star in the constellation Draco
Kepler-90e f g h i Kepler-296b c d e f TOI-1452 b TrES-2b Star clusters LAMOST 1 Nebulae Cat's Eye Nebula NGC 6742 Galaxies NGC 3147 3197 3735 3961 4121
Psi2_Draconis
High-mass X-ray binary
IC 10 X-1 is an X-ray source located in the dwarf galaxy IC 10, an irregular galaxy. It corresponds to a high-mass X-ray binary in which the normal star
IC_10_X-1
Unconfirmed potentially habitable exoplanet
parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra". Astronomy and Astrophysics. 594: A39. arXiv:1606
KOI-4878.01
White-hued chemically unusual star in the constellation Draco
projected rotational velocity of 120 km/s. The star has 1.56 times the mass of the Sun and 1.50 times the Sun's radius. It is radiating 5.75 times the
8_Draconis
Star in the constellation Draco
Astrophysical formulae, Astronomy and astrophysics library, vol. 1 (3rd ed.), Birkhäuser, ISBN 3-540-29692-1. The radius (R*) is given by: 2 ⋅ R ∗ = ( 70.2 ⋅ 0.427
Pi_Draconis
Neutron star
3XMM J004232.1+411314 is a low-mass X-ray binary hosted in the galaxy M31. It is the most luminous source of hard X-rays in the Andromeda Galaxy. It is
3XMM_J004232.1+411314
Blue supergiant star in the constellation Leo
LS1 & 2), at approximately 14 billion light-years from Earth (redshift z=1.49; comoving distance of 14.4 billion light-years; lookback time of 9.34 billion
Icarus_(star)
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
Galaxy containing the Solar System
using LAMOST, SDSS/SEGUE, and Gaia : 3D spherical Jeans equation and tracer mass estimator". Monthly Notices of the Royal Astronomical Society. 516 (1): 731–748
Milky_Way
X-ray binary in Galaxy NGC 300
NGC 300 X-1 is a high mass X-ray binary system located in the spiral galaxy NGC 300, approximately 6 million light-years away in the constellation of
NGC_300_X-1
Star system in the Ursa Major
Qingfeng (2024). "Magnetic Activity of Millions of G-type Stars Based on the LAMOST DR10 Low-resolution Spectral and TESS Light-curve Surveys and the Future
TYC_3801-1529-1
Method in astronomy
Multi-Object Fibre Spectroscopic Telescope (LAMOST) can move the fibers to desired position. The LAMOST moves its 4000 fibers separately within designated
Multi-Object_Spectrometer
G5V star in the constellation Cygnus
Yue; Dong, Subo; Xie, Ji-Wei; Zhang, Wei; Hou, Yonghui; LAMOST-Kepler Collaboration (2018). "LAMOST Observations in the Kepler Field. II. Database of the
Kepler-223
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
Star in the constellation Andromeda
"Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys". The Astrophysical Journal Supplement
KELT-1
Observed discrepancy in galactic angular momenta
using LAMOST, SDSS/SEGUE, and Gaia : 3D spherical Jeans equation and tracer mass estimator". Monthly Notices of the Royal Astronomical Society. 516 (1): 731–748
Galaxy_rotation_curve
Double star in the constellation Draco
spacecraft suggested a central red dwarf with a mass of 0.65 M☉, a radius of 1.1 R☉, and a temperature of 3,639 K (3,366 °C; 6,091 °F). Its candidate exoplanet
KOI-256
Array of smaller mirrors designed to act as one large curved mirror
consists of 91 hexagonal mirror segments, each 1 meter across, resulting in a total hexagonal mirror of 11.1 m by 9.8 m. It is located close to the town
Segmented_mirror
Planet smaller than Neptune with a low density envelope
Kepler Planetary Systems as a Function of Kinematic Age Revealed by the LAMOST–Gaia–Kepler Sample". The Astronomical Journal. 166 (6). American Astronomical
Sub-Neptune
Observatory
60/90 cm Schmidt telescope; a 1.26-meter infrared telescope; and a 2.16-meter telescope. The most recent telescope is the 4m LAMOST. As of 2014 the observatory
Xinglong_Station_(NAOC)
Distant star or star cluster
a single object. The previous farthest known star, MACS J1149 Lensed Star 1, also known as Icarus, at a comoving distance of 14.4 billion light-years
Earendel (astronomical object)
Earendel_(astronomical_object)
Something that has mass and volume
using LAMOST, SDSS/SEGUE, and Gaia : 3D spherical Jeans equation and tracer mass estimator". Monthly Notices of the Royal Astronomical Society. 516 (1): 731–748
Matter
Theoretical cosmological structure
using LAMOST, SDSS/SEGUE, and Gaia : 3D spherical Jeans equation and tracer mass estimator". Monthly Notices of the Royal Astronomical Society. 516 (1): 731–748
Dark_matter_halo
Binary star in the constellation Dorado
discovered four red supergiants in the massive super star cluster Westerlund 1 in the constellation Ara, notably including W26. In 1986, infrared observations
WOH_G64
from the original on 10 March 2025. Retrieved 16 December 2017. "Alcor". LAMOST. Retrieved 19 December 2018. ρ Oph is both the 4th and the 9th additional
List_of_Chinese_star_names
Star in the constellation Draco, orbited by eight planets
Y. (2016). "LAMOST Observations in the Kepler Field: Spectral Classification with the MKCLASS Code". The Astronomical Journal. 151 (1): 13. Bibcode:2016AJ
Kepler-90
List from the Alphabet Direction (αβ)
stars. LAMOST — Large Sky Area Multi-Object Fibre Spectroscopic Telescope (Guo Shoujing Telescope) Latham — David Latham (for example: Latham 1 at 13:10:50
List of astronomical catalogues
List_of_astronomical_catalogues
Long and elongated structure of stars
studied extensively using data from surveys and instruments such as GAIA, LAMOST, 2MASS, SDSS, and more. In 2006, Belokurov and collaborators found that
Sagittarius_Stream
Chinese amateur astronomer (born 1969)
153P/Ikeya-Zhang was discovered by his self-made telescope on February 1, 2002. http://comet.lamost.org/comet/zhang.htm (in Chinese) Portals: Astronomy Biography
Zhang_Daqing
Grand-design spiral galaxy
5383 is interacting with three known galaxies, UGC 8877, LAMOST J135707.72+415027.2, and LAMOST J135700.66+415114.9. One of these galaxies, UGC 8877 is
NGC_5383
Supernova in the constellation Dorado
134440 HE 0437−5439 Holmberg IX V1 IC 10 X-1 Icarus LAMOST J112456.61+453531.3 M51-ULS-1 N6946-BH1 NGC 300 X-1 NGC 2363-V1 NGC 6822-WR 12 SDSS J0715-7334
Sanduleak_−69_202
Star in the Sunburst galaxy
the Sunburst arc". Monthly Notices of the Royal Astronomical Society. 499 (1): L67–L71. arXiv:2004.08400. Bibcode:2020MNRAS.499L..67V. doi:10.1093/mnrasl/slaa163
Godzilla_(star)
Study of the movement of stars
distant hypervelocity star candidates are more promising. In March 2019, LAMOST-HVS1 was reported to be a confirmed hypervelocity star ejected from the
Stellar_kinematics
Binary star system in the constellation Cygnus
parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra". Astronomy and Astrophysics. 594. arXiv:1606.09149
Kepler-16
Wolf–Rayet star in the constellation Dorado
interferometry technique, R136a was shown to be made up of 8 stars within 1 arcsecond at the centre of the cluster, with R136a1 being the brightest. Final
R136a1
European space observatory for astrometry (2013–2025)
distribution within the Milky Way was constructed using data from Gaia and LAMOST spectral survey and machine learning. GaiaNIR (Gaia Near Infra-Red) is a
Gaia_(spacecraft)
Observatory
16-metre reflector telescope (China's largest), and a 1.26-m infrared telescope. The planned "LAMOST", or Large Sky Area Multi-Object Fiber Spectroscopic
Beijing Astronomical Observatory
Beijing_Astronomical_Observatory
List of galactic nuclei
(2010). "A very bright i=16.44 quasar in the 'redshift desert' discovered by LAMOST". Research in Astronomy and Astrophysics. 10 (8): 737. arXiv:1005.5499.
List_of_quasars
Microlensing event in the constellation Andromeda
134440 HE 0437−5439 Holmberg IX V1 IC 10 X-1 Icarus LAMOST J112456.61+453531.3 M51-ULS-1 N6946-BH1 NGC 300 X-1 NGC 2363-V1 NGC 6822-WR 12 SDSS J0715-7334
PA-99-N2
Type of starburst galaxy
sample of 40 BBs, a much larger sample was acquired using data from the LAMOST DR9 survey. Liu et al. found 270 BBs, as well as GPs and "Purple Grapes"
Blueberry_galaxy
Type of star that is luminous, blue, and variable in brightness
6884 (= R40) AF Andromedae AE Andromedae Var 15 Var A-1 J004526.62+415006.3 J004051.59+403303.0 LAMOST J0037+4016 Var 2 (an extremely hot star showing no
Luminous_blue_variable
Sun-like star in the constellation Cygnus
"Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys". The Astrophysical Journal Supplement
Kepler-51
Star in the constellation Dorado
134440 HE 0437−5439 Holmberg IX V1 IC 10 X-1 Icarus LAMOST J112456.61+453531.3 M51-ULS-1 N6946-BH1 NGC 300 X-1 NGC 2363-V1 NGC 6822-WR 12 SDSS J0715-7334
R136b
Star in the constellation Sagittarius
6822-WR 12 is a WN-type Wolf–Rayet star located in the galaxy NGC 6822, about 1.54 million light years away in the constellation of Sagittarius. NGC 6822-WR
NGC_6822-WR_12
State University Department of Physics & Astronomy. September 1, 2022. Retrieved September 1, 2022. "Twitchell Observatory | MSAD 17". MSAD17.org. Maine
List of astronomical observatories
List_of_astronomical_observatories
Eclipsing binary in the constellation of Leo Minor
"Value-added Catalog of M-giant Stars in LAMOST DR9". The Astrophysical Journal Supplement Series. 266 (1): 4. arXiv:2304.00308. Bibcode:2023ApJS..266
AS_Leonis_Minoris
Possible type of luminous blue compact galaxy
(1): 17. arXiv:2203.04207. Bibcode:2022ApJ...929...50P. doi:10.3847/1538-4357/ac5c4b. Li Yuan (30 March 2022). "Compact galaxies discovered by LAMOST"
Pea_galaxy
General map or image of a region of the sky with no specific observational target
galaxies (2014) Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) – an extra-galactic and stellar spectroscopic survey IPHAS and VPHAS+ –
Astronomical_survey
Wolf Rayet star in the constellation Dorado
and another WO star LMC195-1. The two WO stars are only 9" apart. WO stars are classified on the basis of OVI emission at 381.1-383.4 nm, which is weak or
LH_41-1042
Binary star in the constellation Lynx
Identified from the Low-resolution Spectra of LAMOST". The Astrophysical Journal Supplement Series. 277 (1): 15. arXiv:2411.03994. Bibcode:2025ApJS..277
XO-5
Star
"Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys". The Astrophysical Journal Supplement
Kepler-160
Strong explosion observed on stars
Only five of the 34 could be described as fast rotators. Observations from LAMOST have been used to measure chromospheric activity of 5,648 solar-like stars
Superflare
Contact binary star system in the constellation Dorado
134440 HE 0437−5439 Holmberg IX V1 IC 10 X-1 Icarus LAMOST J112456.61+453531.3 M51-ULS-1 N6946-BH1 NGC 300 X-1 NGC 2363-V1 NGC 6822-WR 12 SDSS J0715-7334
VFTS_352
Massive blue supergiant star in the constellation Dorado
134440 HE 0437−5439 Holmberg IX V1 IC 10 X-1 Icarus LAMOST J112456.61+453531.3 M51-ULS-1 N6946-BH1 NGC 300 X-1 NGC 2363-V1 NGC 6822-WR 12 SDSS J0715-7334
Melnick_42
Seyfert 1 galaxy located in the constellation Canes Venatici
IRAS 14026+4341 is a Seyfert type 1 galaxy located in the constellation of Canes Venatici. The redshift of the object is (z) 0.322 and it was first discovered
IRAS_14026+4341
Planetary nebula in the constellation Pegasus
(2019). "Hot Subdwarf Stars Observed in Gaia DR2 and LAMOST DR5". The Astrophysical Journal. 881 (1): 16 pages. arXiv:1906.09393. doi:10.3847/1538-4357/ab298d
NGC_7094
Parameters characterizing properties of our galaxy
using LAMOST, SDSS/SEGUE, and Gaia : 3D spherical Jeans equation and tracer mass estimator". Monthly Notices of the Royal Astronomical Society. 516 (1): 731–748
Oort_constants
Star in the constellation Dorado
into 8 components. R136a2 was marginally the second brightest found within 1 arc-second at the centre of the R136 cluster. Previous estimates that the
R136a2
Eclipsing binary in the constellation Cygnus
Y. (2016). "LAMOST Observations in the Kepler Field: Spectral Classification with the MKCLASS Code". The Astronomical Journal. 151 (1): 13. Bibcode:2016AJ
KIC_9970396
Open cluster in the constellation Taurus
"NGC 1647: A young open cluster with a broad main sequence observed with LAMOST". Astronomy & Astrophysics. 710: A164. arXiv:2604.11765. Bibcode:2026A&A
NGC_1647
O-type main sequence star in the constellation Dorado
134440 HE 0437−5439 Holmberg IX V1 IC 10 X-1 Icarus LAMOST J112456.61+453531.3 M51-ULS-1 N6946-BH1 NGC 300 X-1 NGC 2363-V1 NGC 6822-WR 12 SDSS J0715-7334
BI_253
Hypervelocity star in the constellation Dorado
Astrophysical Journal Letters. 719 (1): L23–L27. arXiv:1007.3493. Bibcode:2010ApJ...719L..23B. doi:10.1088/2041-8205/719/1/L23. S2CID 55832434. "Star on the
HE_0437−5439
Seyfert galaxy located in the constellation of Pisces
PG 0052+251 is a Seyfert type 1 galaxy located in the constellation of Pisces. Its redshift is (z) 0.154 estimating it to be two billion light-years away
PG_0052+251
Binary star system in the constellation Leo Minor
"Value-added Catalogs of M-type Stars in LAMOST DR5". The Astrophysical Journal Supplement Series. 244 (1): 8. arXiv:1908.01128. Bibcode:2019ApJS..244
HD_87822
Main sequence star in constellation of Lyra
"Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys". The Astrophysical Journal Supplement
Kepler-174
Triple star system in Cygnus
parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra". Astronomy and Astrophysics. 594. arXiv:1606.09149
KOI-5
G-type main sequence star in the constellation Ursa Major
Lu, Hongpeng (2025). "Magnetic Activity of TESS Objects Observed in the LAMOST Medium-resolution Spectral Survey". The Astrophysical Journal Supplement
HAT-P-13
Small Magellanic Cloud star in the constellation Tucana
The Astrophysical Journal. 788 (1): 48. arXiv:1310.2241. Bibcode:2014ApJ...788...48S. doi:10.1088/0004-637X/788/1/48. S2CID 119113433. Tabernero, Hugo
HV_2112
Solitary star in the constellation Ursa Major
Astrophysical formulae, Astronomy and astrophysics library, vol. 1 (3rd ed.), Birkhäuser, ISBN 3-540-29692-1. The radius (R*) is given by: 2 ⋅ R ∗ = ( 159.7 ⋅ 2.67
Sigma1_Ursae_Majoris
Star in the constellation Dorado
young star clusters". Monthly Notices of the Royal Astronomical Society. 458 (1): 624–659. arXiv:1603.04994. Bibcode:2016MNRAS.458..624C. doi:10.1093/mnras/stw273
R136a3
Star in the constellation Dorado
B0525-66". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 1 March 2018. On the persistent X-ray emission from the soft gamma-ray repeaters
SGR_0526−66
Gravitationally lensed quasar located in constellation Ursa Major
located in the constellation of Ursa Major. The redshift of the object is (z) 1.841 and was discovered in March 2005 by Masamune Oguri during the Sloan Digital
SDSS_J1001+5027
Star in the constellation Dorado
Large Magellanic Cloud". Astronomy and Astrophysics Supplement Series. 137 (1): 117–145. Bibcode:1999A&AS..137..117B. doi:10.1051/aas:1999240. Woosley,
BAT99-98
as "sassy neighbors" and "scared brothers on police shows". Another time Lamost hosted a "Miss Black USA" pageant hosted by a ghetto area of an unnamed
List of In Living Color sketches
List_of_In_Living_Color_sketches
Star in the constellation Cygnus
"Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys". The Astrophysical Journal Supplement
PH2
Cloud of gas or a trail around a comet or asteroid
2023-07-30. "Chapter 14, Section 2 | Comet appearance and structure". lifeng.lamost.org. Retrieved 2017-01-08. "comet". Dictionary.com Unabridged (Online).
Coma_(comet)
Star in Large Magellanic Cloud
134440 HE 0437−5439 Holmberg IX V1 IC 10 X-1 Icarus LAMOST J112456.61+453531.3 M51-ULS-1 N6946-BH1 NGC 300 X-1 NGC 2363-V1 NGC 6822-WR 12 SDSS J0715-7334
HD_37836
Star in the Triangulum Galaxy
estimated to have a progenitor mass over 40 M☉ and to be losing mass at a rate of 1 M☉ every 25,000–50,000 years. The mass loss is highest when the star is largest
Romano's_Star
travel, tourism, insurance
LAMOST 1
LAMOST 1
LAMOST 1
LAMOST 1
LAMOST 1
LAMOST 1
LAMOST 1
LAMOST 1
LAMOST 1
travel, tourism, insurance