The companion of Mira Ceti - A possible source of soft X-rays

Details The companion of Mira Ceti - A possible source of soft X-rays The companion of Mira Ceti - A possible source of soft X-rays

Sep 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976pazh....2..425s&link_type=associated

Pis'ma v Astronomicheskii Zhurnal, vol. 2, Sept. 1976, p. 425, 426. In Russian.

Astronomy and Astrophysics

Astrophysics

Companion Stars, Giant Stars, Mira Variables, Stellar Temperature, White Dwarf Stars, X Ray Sources, Astrophysics, Stellar Luminosity, Stellar Mass Ejection, Variable Stars

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