Computer Science
Scientific paper
Apr 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987aipc..155...83s&link_type=abstract
AIP Conference Proceedings, Volume 155, pp. 83-86 (1987).
Computer Science
2
Scientific paper
We have obtained high-resolution 2-μm spectra of six late-type stars within 2 pc of the Galactic Center. We have derived spectral types, reddenings, and radial velocities for these stars. We find the supergiant density in the Galactic Center is lower than in previous determinations. No correspondence is found between stellar velocities and Ne II velocities observed along the same line of sight. No systematic rotation or ordered motion is seen in the stellar velocity distribution. The mass distribution derived from the stellar velocities is compared to those derived from gas velocities and from the 2-μm light.
Hall Donald N. B.
Kleinmann Susan G.
Scoville Nicholas Z.
Sellgren Kris
No associations
LandOfFree
Kinematics of individual stars in the Galactic Center does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Kinematics of individual stars in the Galactic Center, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Kinematics of individual stars in the Galactic Center will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1346974