HD 51956 - A supergiant in an interacting binary

Details HD 51956 - A supergiant in an interacting binary HD 51956 - A supergiant in an interacting binary

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...364l..13p&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 364, Nov. 20, 1990, p. L13-L15.

Astronomy and Astrophysics

Astrophysics

2

Binary Stars, Companion Stars, Hot Stars, Supergiant Stars, Ultraviolet Spectra, Variable Stars, B Stars, High Temperature Plasmas, Iue

Scientific paper

IUE ultraviolet spectral observations reveal that the F supergiant HD 51956 contains a hot companion star partially obscured by warm plasma. Variable absorption features are analogous to those in the strongly interacting system HD 207739. The F type component is apparently transferring matter to a subluminous B type star which originally was the primary component.

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