Dictionary of Nomenclature of Celestial Objects

 he inner radius of the    annulus in which the star lies.
The number following the hyphen is ordered in the sense of increasing distance from Sgr A* within each annulus.
See also [EG97], [GEO97], [PGM2006], [RGH2007]. in source:NAME Gal Center Ref:=1998ApJ...509..678G byGHEZ A.M. , KLEIN B.L., MORRIS M., BECKLIN E.E. Astrophys. J., 509, 678-686 (1998) High proper-motion stars in the vicinity of Sagittarius A* evidence for a supermassive black hole at the center of our galaxy. ocross-id.: WNN = [GEO97] WNN, SNN = [EG97] SNN, NNA or NNWW = GCIRS NNA or NNWW oTable 1: <[GKM98] S0-NN> (Nos S0-1 to S0-15), <[GKM98] S1-NN> (Nos S1-1 to S1-15, <[GKM98] S2-NN> (Nos S2-1 to S2-32), <[GKM98] S3-NN> (Nos S3-1 to S3-13), <[GKM98] S4-N> (Nos S4-1 to S4-5). Ref:=2002ApJ...576..790G byGEZARI S. , GHEZ A.M., BECKLIN E.E., LARKIN J., McLEAN I.S., MORRIS M. Astrophys. J., 576, 790-797 (2002) Adaptive optics near-infrared spectroscopy of the Sagittarius A* cluster. oTable 1, Fig.2: <[GKM98] S0-NN> (Nos S0-16 to S0-18) added. Ref:=2003S&T...105d..44T byTANNER A. Sky Telesc., 105, part no 4, 44-50 (2003) A trip to the Galactic Center. oFig.p.49: <[GKM98] SN-NN> (Nos S0-19, S0-20) added. Ref:=2005ApJ...620..744G byGHEZ A.M. , SALIM S., HORNSTEIN S.D., TANNER A., LU J.R., MORRIS M., BECKLIN E.E., DUCHENE G. Astrophys. J., 620, 744-757 (2005) Stellar orbits around the Galactic Center black hole. oTable 1: <[GKM98] SN-NN> (Nos S0-21 to S0-26) added. Ref:=2007ApJ...659.1241R byRAFELSKI M. , GHEZ A.M., HORNSTEIN S.D., LU J.R., MORRIS M. Astrophys. J., 659, 1241-1256 (2007) Photometric stellar variability in the Galactic Center. oTables 2, 3, col(1): <[GKM98] SN-NN> N=69 added among (Nos S0-27 to S0-36, S1-17 to S1-68, S2-34 to S2-86, S3-16). Tables 2, 3, col(2): <[RGH2007] GEN+x.xx+y.yy> N=26. Ref:=2007ApJ...667..900H byHORNSTEIN S.D. , MATTHEWS K., GHEZ A.M., LU J.R., MORRIS M., BECKLIN E.E., RAFELSKI M., BAGANOFF F.K. Astrophys. J., 667, 900-910 (2007) A constant spectral index for Sagittarius A* during infrared/X-ray intensity variations. oFig.3: <[GKM98] S0-NN> (No. S0-37) added. Ref:=2009ApJ...691.1021D byDO T. , GHEZ A.M., MORRIS M.R., YELDA S., MEYER L., LU J.R., HORNSTEIN S.D., MATTHEWS K. Astrophys. J., 691, 1021-1034 (2009) A near-infrared variability study of the Galactic black hole: a red noise source with NO detected periodicity. oFig.1: <[GKM98] SN-NNN> (Nos S0-38, S2-42, S2-133) added. Ref:=2010ApJ...725..331Y byYELDA S. , LU J.R., GHEZ A.M., CLARKSON W., ANDERSON J., DO T., MATTHEWS K. Astrophys. J., 725, 331-352 (2010) Improving Galactic Center astrometry by reducing the effects of geometric distortion. o(Erratum) erratum vol. 726, p. 114 (2011) oTable 7: <[GKM98] S0-NNN> (Nos S0-53) added, <[GKM98] S1-NNN> (Nos S1-167) added, <[GKM98] S2-NNN> N=9 among (Nos S2-134 to S2-319) added, <[GKM98] S3-NNN> N=81 among (Nos S3-17 to S3-390) added, <[GKM98] S4-NNN> N=77 among (Nos S4-6 to S4-372) added, <[GKM98] S5-NNN> N=86 among (Nos S5-6 to S5-258), <[GKM98] S6-NNN> N=123 among (Nos S6-0 to S6-176), <[GKM98] S7-NNN> N=98 among (Nos S7-3 to S7-103), <[GKM98] S8-NNN> (Nos S8-1 to S8-114), <[GKM98] S9-NNN> (Nos S9-1 to S9-108),<[GKM98] S10-NNN> (Nos S10-1 to S10-95), <[GKM98] S11-NNN> (Nos S11-1 to S11-85), <[GKM98] S12-NNN> (Nos S12-1 to S12-64), <[GKM98] S13-NNN> (Nos S13-1 to S13-60), <[GKM98] S14-NNN> (Nos S14-1 to S14-56), <[GKM98] S15-NNN> (Nos S15-1 to S15-35), <[GKM98] S16-NNN> (Nos S16-1 to S16-18), <[GKM98] S17-NNN> N=10 among (Nos S17-2 to S17-11), <[GKM98] S18-NNN> (Nos S18-1 to S18-3). Ref:=2013ApJ...764..154D byDO T. , LU J.R., GHEZ A.M., MORRIS M.R., YELDA S., MARTINEZ G.D., WRIGHT S.A., MATTHEWS K. Astrophys. J., 764, 154 (2013) Stellar populations in the central 0.5 pc of the galaxy. I. A new method for constructing luminosity functions and surface-density profiles. oTables 2-3: <[GKM98] S2-NNN> (Nos S2-317 and S2-319) added, <[GKM98] S6-NNN) (No S6-181) added, <[GKM98] S7-NNN> (No S7-104) added, <[GKM98] S8-NNN> (No S8-124) added, <[GKM98] S11-NNN> (Nos S11-86 and S11-88) added. Ref:=2013ApJ...779L...6D byDO T. , MARTINEZ G.D., YELDA S., GHEZ A., BULLOCK J., KAPLINGHAT M., LU J.R., PETER A.H.G., PHIFER K. Astrophys. J., 779L, 6 (2013) Three-dimensional stellar kinematics at the Galactic Center: measuring the nuclear star cluster spatial density profile, black hole mass, and distance. oTable 1: <[GKM98] S2-NNN> (Nos S2-308 and S2-317) added, <[GKM98] S6-NNN) (No S6-181) added, <[GKM98] S7-NNN> (No S7-104) added, <[GKM98] S8-NNN> (Nos S8-119, S8-121, S8-124) added, <[GKM98] S10-NNN> N=5 (Nos S10-96 to S10-99, S10-100 to S10-102) added, <[GKM98] S11-NNN> (Nos S11-86 and S11-88) added, <[GKM98] S12-NNN> N=7 among (Nos S12-67 to S12-75) added. Ref:=2016ApJ...830...17B byBOEHLE A. , GHEZ A.M., SCHODEL R., MEYER L., YELDA S., ALBERS S., MARTINEZ G.D., BECKLIN E.E., DO T., LU J.R., MATTHEWS K., MORRIS M.R., SITARSKI B., WITZEL G. Astrophys. J., 830, 17-17 (2016) An improved distance and mass estimate for Sgr A* from a multistar orbit analysis. oTable 6: <[GKM98] S6-NNN> (Nos S6-182 to S6-185) added, <[GKM98] S7-NNN> (Nos S7-112 and S7-114) added, <[GKM98] S8-NNN> (Nos S8-125 to S8-130) added, <[GKM98] S9-NNN> N=9 among (Nos S9-117 to S9-293) added, <[GKM98] S10-NNN> N=7 among (Nos S10-096 to S10-113) added, <[GKM98] S11-NNN> N=4 among (Nos S11-93 to S11-98) added, <[GKM98] S12-NNN> N=6 among (Nos S12-076 to S12-129) added, <[GKM98] S13-NNN> N=4 among (Nos S13-065 to S13-068) added, <[GKM98] S14-NNN> N=3 among (Nos S14-058 to S14-177) added, <[GKM98] S15-NNN> N=3 among (Nos S15-038 to S15-042) added, <[GKM98] S17-NNN> (No S17-013) added. =E=Catalogue in electronic form as J/ApJ/659/1241 =E=Catalogue in electronic form as <J/ApJ/764/154/>
====Sorry, no entry could be found====

© Université de Strasbourg/CNRS

    • Contact