Discovery of multiple low-luminosity X-ray sources in NGC 6397

Details Discovery of multiple low-luminosity X-ray sources in NGC 6397 Discovery of multiple low-luminosity X-ray sources in NGC 6397

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...410l.103c&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 410, no. 2, p. L103-L106.

Astronomy and Astrophysics

Astrophysics

48

Binary Stars, Globular Clusters, Rosat Mission, Stellar Luminosity, X Ray Stars, Cataclysmic Variables, X Ray Sources

Scientific paper

New low-luminosity X-ray sources have been discovered in NGC 6397 with
the ROSAT High Resolution Imager. These sources have a total number,
spatial distribution, and X-ray luminosities consistent with their being
CVs. The findings supports the hypothesis that the low-luminosity X-ray
sources in clusters are generally dominated by CVs.

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