Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988baicz..39..296h&link_type=abstract
Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 39, no. 5, 1988, p. 296-302.
Astronomy and Astrophysics
Astronomy
1
Astronomical Photometry, Flare Stars, Visible Spectrum, X Ray Sources, Brightness Distribution, Exosat Satellite, Light Curve, Luminosity, Photosphere
Scientific paper
Results of the Exosat X-ray observations and quasi-simultaneous optical photographic photometry of the X-ray source EXO 020528 + 1454.8 = 1 E 0205 + 149 are presented and discussed. The results indicate that the source is identical to the Lowell proper motion object G 035 - 027, a pair in which at least one but more probably both members are dMe flaring stars. The integral X-ray luminosity is between about 1.8 x 10 to the 28th and 5.3 x 10 to the 29th erg/s for the pair or about 9 x 10 to the 27th to 4 x 10 to the 28th erg/s for each component. The object shows a soft X-ray spectrum with a blackbody temperature of about 10 to the 6th K, X-ray variability of a factor of about three over time intervals of months to years, X-ray to bolometric luminosity ratio of about 0.0001 to 0.001 indicating flaring activity, and possible optical flares with amplitudes of the order of one magnitude or larger in B on at least one component of the star system.
Goetz Walter
Hacke G.
Hudec Rene
Huth Hans
Lovas M.
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