Coronal X rays from single, magnetic white dwarfs - A search and probable detection

Details Coronal X rays from single, magnetic white dwarfs - A search and probable detection Coronal X rays from single, magnetic white dwarfs - A search and probable detection

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992pasp..104..239a&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 104, no. 674, April 1992, p. 239-241.

Other

8

Cool Stars, Magnetic Stars, Stellar Coronas, Stellar Radiation, White Dwarf Stars, X Ray Sources, Bremsstrahlung, Heao 2, Stellar Envelopes, Stellar Luminosity

Scientific paper

X-ray emission from a sample of five nearby (6-20 pc), strongly magnetic (10-200 MG), relatively cool (6000-14,000 K), single white dwarfs, two of which may possess coronae was explored. One star (GR 290) at better than 99-percent confidence is detected and upper limits from Einstein Observatory IPC data for four others are given. The detected luminosities and limits are in the range 1.4-12.5 x 10 exp 27 ergs/s.

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