X-ray emission from the W UMa system TZ Bootis

Details X-ray emission from the W UMa system TZ Bootis X-ray emission from the W UMa system TZ Bootis

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..97..225g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 97, no. 2, Dec. 1983, p. 225-227. Research supported by the Bundesminister

Astronomy and Astrophysics

Astronomy

Eclipsing Binary Stars, Stellar Radiation, X Ray Sources, Heao 2, Stellar Luminosity, X Ray Astronomy

Scientific paper

HEAO-B (Einstein) satellite measurements with the Imaging Proportional
Counter revealed the W UMa binary system TZ Bootis as an X-ray source.
It is estimated that the luminosity ratio Lx/LV of
this system is about 10-3.8 indicating that TZ Bootis is in
the transition region between A- and W-type W UMa systems.

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