Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ssrv...59....1g&link_type=abstract
Space Science Reviews (ISSN 0038-6308), vol. 59, Jan. 1992, p. 1-81. Research supported by ASI.
Astronomy and Astrophysics
Astronomy
63
B Stars, Early Stars, Stellar Flares, Stellar Spectra, X Ray Binaries, X Ray Spectra, Emission Spectra, Infrared Astronomy, Neutron Stars, Stellar Mass, Stellar Winds, Ultraviolet Astronomy
Scientific paper
A review of the principal characteristics and behavior of the X-ray/Be system A 0535 + 26/HDE 245770, emphasizing the morphological and physical aspects, is presented. The binary system is formed by a O9.7IIIe star that acts as a 'normal' Be star and by a neutron star, which is a slow X-ray pulsar (104s). Based on the behavior of the binary system, derived mainly from simultaneous multifrequency measurements showing differences in intensity of the X-ray outbursts and in repetition time and activity of the Be star, three types of X-ray outbursts related to the variable activity of the Be star are established.
Giovannelli Franco
Graziati Lola S.
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