Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...287..586b&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 287, Dec. 15, 1984, p. 586-609. Research supported by the University of Cal
Astronomy and Astrophysics
Astrophysics
471
Abundance, Andromeda Galaxy, Astronomical Spectroscopy, Elliptical Galaxies, Galactic Clusters, Galactic Nuclei, Globular Clusters, Absorption Spectra, Balmer Series, Iue, Metallicity, Wavelengths
Scientific paper
Integrated 9 A-resolution spectra in the 4000-6300 A region are presented for 17 Galactic globular clusters and 19 M31 globular clusters. Indices for 11 molecular bands and lines and several broadband colors are compared between the M31 and galactic cluster systems, as well as with the nuclei of 170 E galaxies. H-beta and CN are noted to differ markedly among the three groups. It is suggested that the three old stellar populations presently examined must differ in one or more respects beyond mean metallicity. Several models are analyzed to account for the higher H-beta and CN in M31 globulars. Most models fail to yield the requisite simultaneous H-beta and CN enhancements, except perhaps those of younger age. Satellite UV flux measurements will eventually offer an important tool for discriminating between various possible warm star components.
Burstein David
Faber Sandra M.
Gaskell Martin C.
Krumm Nathan
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