On the stellar content of the galactic globular cluster M5

Details On the stellar content of the galactic globular cluster M5 On the stellar content of the galactic globular cluster M5

Feb 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...118..332a&link_type=abstract

Astronomy and Astrophysics, vol. 118, no. 2, Feb. 1983, p. 332-336.

Astronomy and Astrophysics

Astronomy

3

Globular Clusters, Stellar Spectra, Ultraviolet Astronomy, Astronomical Models, Dwarf Stars, Giant Stars, Iue, Wavelengths

Scientific paper

New IUE observations of the innermost region of the galactic globular cluster M5 (NGC 5904) are presented and discussed. Addition of IUE spectra and identification of spectral features were obtained from the present and previous IUE observations of M5. Synthetic models of the cluster were constructed by taking into account optical and UV data. A comparison between theory and observation allowed for some estimates of the stellar content of M5. However, attention is called to the limits of validity of synthetic models, at least when they are compared with IUE observations.

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