Coordinated ROSAT and speckle observations of the Mira AB system

Details Coordinated ROSAT and speckle observations of the Mira AB system Coordinated ROSAT and speckle observations of the Mira AB system

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996sao..reptq....k&link_type=abstract

Technical Report, Smithsonian Astrophysical Observatory Cambridge, MA United States

Astronomy and Astrophysics

Astrophysics

Rosat Mission, Speckle Interferometry, Iue, X Rays, Main Sequence Stars, Estimating, Luminosity, Spectra

Scientific paper

ROSAT observations of the Mira AB system carried out using PSPC resulted in an unambiguous detection of Mira B at x-ray wavelengths. Coordinated observations were carried out using various techniques including IUE and speckle interferometry. We estimated the x-ray luminosity associated with the accretion component using several spectral models. Our results suggest that Mira B could be a main sequence star. The system was resolved using speckle observations and we determined the distance and the magnitude difference between the components.

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