[GKM98] S2-66 , the SIMBAD biblio

[GKM98] S2-66 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST05:46:04


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Title First 3 Authors
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.
2009ApJ...690.1463L 129       D     X   F     3 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...499..483B viz 39           X         1 30 162 Composition of the Galactic center star cluster. Population analysis from adaptive optics narrow band spectral energy distributions. BUCHHOLZ R.M., SCHOEDEL R. and ECKART A.
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.
2013ApJ...764..154D viz 15       D               1 307 105 Stellar populations in the central 0.5 pc of the galaxy. I. A new method for constructing luminosity functions and surface-density profiles. DO T., LU J.R., GHEZ A.M., et al.
2014ApJ...786L..12G 15       D               1 30 39 Possible origin of the G2 cloud from the tidal disruption of a known giant star by Sgr A*. GUILLOCHON J., LOEB A., MacLEOD M., 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 81           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.
2023ApJ...949...18J viz 44           X         1 183 ~ Stellar Populations in the Central 0.5 pc of Our Galaxy. III. The Dynamical Substructures. JIA S., XU N., LU J.R., et al.

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