X-ray to infrared observations of the AM Herculis system E1405 - 451 (V834 Centauri)

Details X-ray to infrared observations of the AM Herculis system E1405 - 451 (V834 Centauri) X-ray to infrared observations of the AM Herculis system E1405 - 451 (V834 Centauri)

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...374..744s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 374, June 20, 1991, p. 744-752.

Astronomy and Astrophysics

Astronomy

7

Centaurus Constellation, Infrared Astronomy, Spaceborne Astronomy, X Ray Astronomy, X Ray Binaries, Exosat Satellite, Iue, Ultraviolet Spectra

Scientific paper

The Exosat satellite observed E1405 - 451 in the X-ray band in March 1984 during a high state; and simultaneous UV, optical, and IR coverage was obtained with IUE and from ESO telescopes. The low-energy X-ray curve exhibits a minimum at phase zero which is similar to the optical one, with some indication of temperature modulation with orbital phase. On the contrary, the medium-energy X-ray curve exhibits a broad minimum at phase zero, and the column density varies with phase, which may account for the entire modulation of the intensity.

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