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A New Method for Measuring the Detailed Chemical Composition of Globular Clusters from High-Resolution, Integrated-Light Spectra

Published online by Cambridge University Press:  03 August 2017

Rebecca A. Bernstein  and
Andrew McWilliam
Rebecca A. Bernstein
Affiliation:
Carnegie Observatories, 813 Santa Barbara St., Pasadena, CA, 91101
Andrew McWilliam
Affiliation:
Carnegie Observatories, 813 Santa Barbara St., Pasadena, CA, 91101

Abstract

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We are developing a method for measuring the detailed chemical composition and evolutionary history of extragalactic star clusters from high resolution spectra of their integrated light as one would from spectra of individual stars. In this paper, we show high signal-to-noise ratio echelle spectra of the integrated light of two Galactic globular clusters and equivalent-quality spectra of individual stars in those clusters in order to briefly illustrate some subtleties of the analysis method.

Information

Type
Part 4. Star Cluster Formation and Evolution: Theory and Observation
Information
Symposium - International Astronomical Union , Volume 207: Extragalactic Star Clusters , 2002 , pp. 739 - 742
Copyright
Copyright © Astronomical Society of the Pacific 2002 

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