Ejection from pulsars in binary systems

Details Ejection from pulsars in binary systems Ejection from pulsars in binary systems

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss..98..221l&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 98, no. 2, Jan. 1984, p. 221-236.

Astronomy and Astrophysics

Astrophysics

17

Binary Stars, Pulsars, Stellar Mass Ejection, Stellar Models, Mathematical Models, Radio Emission, Stellar Winds

Scientific paper

Interaction of an ejecting pulsar in a binary with the matter surrounding it is considered. Around the pulsar a cavern is formed, and its shape is calculated. The non-stationary regime of 'floating' caverns filled with binary radioemission is discussed. This regime can lead to a special radio-burster. It is noticed that in binaries with rather large separation between components, a pulsed radioemission from a pulsar can be observed. In this case, the pulsar will be a fine probe for exploration of physical characteristics of a stellar wind from a normal expansion.

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