Theoretical constraints on far UV radiation from old Population II stellar systems

Details Theoretical constraints on far UV radiation from old Population II stellar systems Theoretical constraints on far UV radiation from old Population II stellar systems

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26as...59..505c&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 59, March 1985, p. 505-509.

Statistics

Computation

3

Far Ultraviolet Radiation, Globular Clusters, Horizontal Branch Stars, Stellar Radiation, Ultraviolet Astronomy, Computational Astrophysics, Star Distribution, Stellar Temperature

Scientific paper

The UV flux from Population II systems is evaluated on the basis of
globular cluster population distribution, ZAHB structures, and model
atmospheres. The results may be used as constraints in stellar
population analysis when interpreting far UV observations of globular
clusters and galaxies.

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