Ultraviolet fluxes for globular clusters in M31 - A rediscussion

Details Ultraviolet fluxes for globular clusters in M31 - A rediscussion Ultraviolet fluxes for globular clusters in M31 - A rediscussion

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990aj....100..141c&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 100, July 1990, p. 141-145. Research supported by McDonald Observatory and National

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10

Globular Clusters, Radiant Flux Density, Ultraviolet Radiation, Data Acquisition, Data Reduction, Iue, Wavelengths

Scientific paper

Long-exposure observations of three bright globular clusters in M31 obtained with both the short- and long-wavelength low-resolution cameras of the International Ultraviolet Explorer satellite are discussed. All of the clusters are seen at the longer wavelengths, but only one of the clusters is seen at short wavelengths, and this detection is marginal. The ultraviolet fluxes are in fact known with only poor precision, and previous conclusions concerning the stellar population are weakened accordingly. Discrepancies between the ultraviolet fluxes obtained here and in other published work are described.

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