Fourteen years of multifrequency-coordinated observations of the X-ray/Be system A 0535 + 26/HDE 245770

Details Fourteen years of multifrequency-coordinated observations of the X-ray/Be system A 0535 + 26/HDE 245770 Fourteen years of multifrequency-coordinated observations of the X-ray/Be system A 0535 + 26/HDE 245770

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.169..139g&link_type=abstract

(IAU, European Regional Astronomy Meeting on New Windows to the Universe, 11th, La Laguna, Spain, July 3-8, 1989) Astrophysics a

Astronomy and Astrophysics

Astrophysics

4

B Stars, Pulsars, Stellar Mass Accretion, X Ray Stars, Iue, Ultraviolet Spectra

Scientific paper

Within the framework of a very long multifrequency campaign of coordinated, and very often simultaneous, observations of the transient X-ray/Be system A 0535 + 26/HDE 245770, the paper presents a summary of this large collection of data taken with the IUE and ASTRON satellites as well as with many ground-based telescopes in the optical and IR regions. Emphasis is placed here on the physics and dynamics of the mass transfer at periastron and subsequent X-ray flaring, which is a typical problem of the X-ray/Be binary system class.

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