Abstracts, Galactic Center Workshop '98
GCNEWS
A Newsletter for Galactic Center Research
This Volume was edited by Angela Cotera & Heino Falcke
email: gcnews@aoc.nrao.edu

ABSTRACT

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The Stellar Content of the Galactic Center
Blum, R. D.1; Ram\'irez S. V.2; Sellgren, K.,2
1 Cerro Tololo Interamerican Observatory, La Serena, Chile; 2 The Ohio State University, Columbus, OH, USA;
ABSTRACT:
We present H and K band spectra for a nearly complete sample of K-band
bright stars in the central few parsecs of the Milky Way. The sample
is defined as those stars in the Galactic Center (GC) K-band luminosity
function which are brighter than the brightest stars in the Baade's
Window K-band luminosity function. The new spectra of the K-band bright
stars uniformly show CO 2.3 micron absorption, the signature of
luminous, cool stars. Perhaps not surprisingly, it is the
luminous cool stars which dominate the bright end of
GC K-band luminosity function. We compare the atomic and
molecular line strengths of the GC stars to those for nearby and bulge
populations. We also use the GC K-band bright star properties as
derived from their spectra and broad band magnitudes to discuss
implications for recent and past star formation.
LINKS: Program, Author, rblum@noao.edu
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