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- W2034891063 abstract "The expanding atmosphere of the massive close binary DH Cephei is analyzed on the basis of data from ground-based polarimetry and spaceborne UV observations obtained with the IUE satellite. The mass loss from the system is estimated to be about 2 x 10 to the -6th solar mass/yr. This material can be divided into three classes: (1) wind material, which is hot gas driven from the stars via radiation pressure and reaching terminal velocity at a distance of 5a or greater; (2) scattering material, which may be the result of colliding winds or instabilities in the wind flow; and (3) small (0.1 micron) dust grains. The latter may originate in the cold high-density boundary formed as the wind from the binary plows into the ambient interstellar medium or, alternatively, may be the residue of the formation of stellar components." @default.
- W2034891063 created "2016-06-24" @default.
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- W2034891063 date "1991-01-01" @default.
- W2034891063 modified "2023-10-02" @default.
- W2034891063 title "Circumstellar material around the massive close binary DH Cephei" @default.
- W2034891063 doi "https://doi.org/10.1086/169563" @default.
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