Photometric Outbursts in Mira B

Details Photometric Outbursts in Mira B Photometric Outbursts in Mira B

May 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aas...194.6603c&link_type=abstract

American Astronomical Society, 194th AAS Meeting, #66.03; Bulletin of the American Astronomical Society, Vol. 31, p.929

Astronomy and Astrophysics

Astronomy

Scientific paper

Photoelectric photometry of Mira near minimum light show two outbursts of 0.6 mag on a two hour time scale. We construct a three component model for the photometry: Mira A (at minimum light), a white dwarf (Mira B), and accretion material surrounding Mira B. The time scale indicates that accretion processes surrounding Mira B are responsible for the outbursts rather than changes in the stellar wind of Mira A

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