[GEO97] W7 , the SIMBAD biblio

[GEO97] W7 , the SIMBAD biblio (22 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST01:38:01


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Title First 3 Authors
1997MNRAS.291..219G 2 38 345 On the nature of the dark mass in the centre of the Milky Way. GENZEL R., ECKART A., OTT T., et al.
1998ApJ...509..678G 2 85 597 High proper-motion stars in the vicinity of Sagittarius A* evidence for a supermassive black hole at the center of our galaxy. GHEZ A.M., KLEIN B.L., MORRIS M., et al.
2000MNRAS.317..348G 1 95 334 Stellar dynamics in the Galactic Centre: proper motions and anisotropy. GENZEL R., PICHON C., ECKART A., et al.
2006ApJ...643.1011P viz 16       D               119 600 The two young star disks in the central parsec of the Galaxy: properties, dynamics, and formation. PAUMARD T., GENZEL R., MARTINS F., et al.
2006ApJ...648..405B 31 36 Clockwise stellar disk and the dark mass in the Galactic Center. BELOBORODOV A.M., LEVIN Y., EISENHAUER F., et al.
2007ApJ...659.1241R viz 15       D               1 135 26 Photometric stellar variability in the Galactic Center. RAFELSKI M., GHEZ A.M., HORNSTEIN S.D., et al.
2009ApJ...690.1463L 92       D         F     2 48 286 A disk of young stars at the Galactic Center as determined by individual stellar orbits. LU J.R., GHEZ A.M., HORNSTEIN S.D., et al.
2009A&A...502...91S viz 15       D               1 345 213 The nuclear star cluster of the Milky Way: proper motions and mass. SCHOEDEL R., MERRITT D. and ECKART A.
2009ApJ...703.1323D viz 90       D         F     2 194 159 High angular resolution integral-field spectroscopy of the Galaxy's nuclear cluster: a missing stellar cusp? DO T., GHEZ A.M., MORRIS M.R., et al.
2014ApJ...783..131Y viz 15       D               1 130 135 Properties of the remnant clockwise disk of young stars in the Galactic Center. YELDA S., GHEZ A.M., LU J.R., et al.
2015A&A...584A...2F viz 16       D               2 100 41 KMOS view of the Galactic centre. I. Young stars are centrally concentrated. FELDMEIER-KRAUSE A., NEUMAYER N., SCHOEDEL R., et al.
2016ApJ...819...60Y 16       D               1 168 7 Sgr A* and its environment: low-mass star formation, the origin of X-ray gas and collimated outflow. YUSEF-ZADEH F., WARDLE M., SCHODEL R., et al.
2016ApJ...830...17B viz 16       D               1 967 289 An improved distance and mass estimate for Sgr A* from a multistar orbit analysis. BOEHLE A., GHEZ A.M., SCHODEL R., et al.
2019ApJ...871..103G viz 57       D     X         2 62 3 An adaptive optics survey of stellar variability at the Galactic Center. GAUTAM A.K., DO T., GHEZ A.M., et al.
2019ApJ...873...65S viz 16       D               1 614 8 The Galactic Center: an improved astrometric reference frame for stellar orbits around the supermassive black hole. SAKAI S., LU J.R., GHEZ A., et al.
2019ApJ...882L..28C 57       D     X         2 31 ~ Consistency of the infrared variability of Sgr A* over 22 yr. CHEN Z., GALLEGO-CANO E., DO T., et al.
2022ApJ...932L...6V viz 17       D               2 183 18 The Young Stars in the Galactic Center. VON FELLENBERG S.D., GILLESSEN S., STADLER J., et al.
2023ApJ...948...94C viz 17       D               1 58 2 Evidence of a Decreased Binary Fraction for Massive Stars within 20 milliparsecs of the Supermassive Black Hole at the Galactic Center. CHU D.S., DO T., GHEZ A., et al.
2023ApJ...949...18J viz 17       D               3 183 ~ Stellar Populations in the Central 0.5 pc of Our Galaxy. III. The Dynamical Substructures. JIA S., XU N., LU J.R., et al.
2023ApJ...954L..33W 44           X         1 21 ~ Near-infrared Flux Distribution of Sgr A* from 2005-2022: Evidence for an Enhanced Accretion Episode in 2019. WELDON G.C., DO T., WITZEL G., et al.
2024ApJ...964..164G viz 152       D     X         4 393 ~ An Estimate of the Binary Star Fraction among Young Stars at the Galactic Center: Possible Evidence of a Radial Dependence. GAUTAM A.K., DO T., GHEZ A.M., et al.
2024ApJ...977..228P 45           X         1 21 ~ New Evidence for a Flux-independent Spectral Index of Sgr A* in the Near-infrared. PAUGNAT H., DO T., GAUTAM A.K., et al.

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