/ftp/cats/J/ApJ/643//1011



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J/ApJ/643/1011  Properties of central Galaxy early-type stars   (Paumard+, 2006)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	table2.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/ApJ/643/1011
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Beginning of ReadMe : J/ApJ/643/1011 Early-type stars in the center of the Galaxy (Paumard+, 2006) ================================================================================ The two young star disks in the central parsec of the Galaxy: properties, dynamics, and formation. Paumard T., Genzel R., Martins F., Nayakshin S., Beloborodov A.M., Levin Y., Trippe S., Eisenhauer F., Ott T., Gillessen S., Abuter R., Cuadra J., Alexander T., Sternberg A. <Astrophys. J., 643, 1011-1035 (2006)> =2006ApJ...643.1011P ================================================================================ ADC_Keywords: Stars, nearby ; Stars, early-type ; Space velocities Keywords: Galaxy: center - stars: early-type - stars: formation - stars: luminosity function, mass function - stellar dynamics Abstract: We report the definite spectroscopic identification of  40 OB supergiants, giants, and main-sequence stars in the central parsec of the Galaxy. Detection of their absorption lines has become possible with the high spatial and spectral resolution and sensitivity of the adaptive optics integral field spectrometer SPIFFI/SINFONI on the ESO VLT. Several of these OB stars appear to be helium- and nitrogen-rich. Description: Data are from various data sets we have been able to obtain with both SPIFFI as a guest instrument (in 2003) and SINFONI during its commissioning in 2004 and guaranteed time observation (GTO) runs in 2005. These data have been taken in the K band with a resolution R=4000 (FWHM=85km/s) and in the H+K mode (R=1500, FWHM=230km/s). Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 17 45 40.0 -29 00 28 Galactic Center = Gal 000.0+00.0 ----------------------------------------------------------