Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 2012
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012astbu..67...44b&link_type=abstract
Astrophysical Bulletin, Volume 67, Issue 1, pp.44-56
Astronomy and Astrophysics
Astrophysics
Stars: Magnetic, Stars: Binaries, Methods: Observational: Speckle Interferometry
Scientific paper
We present the results of speckle interferometry of a sample of 117 chemically peculiar stars with global magnetic fields. The observations were made in December 2009 at the BTA with a spatial resolution of about 0.02″ in the visual spectral region. Twenty-nine stars were resolved into individual components, 14 of them for the first time (HD965, HD5797, HD8855, HD10783, HD16605, HD21699, HD35502, HD51418, HD64486, HD79158, HD103498, HD108651, HD213918, HD293764). In twelve cases a companion turned out to be 2-4 m fainter than the main component—a magnetic star. Young hot Bp stars HD35502 and HD213918 are exceptions, since their companions are fainter by about 1 m . In all cases, the linear distance from a star to its companion at the epoch of observations in the picture plane exceeded 109 km. Eighty-eight magnetic CP stars revealed no secondary components within our study. Thus, the fraction of speckle interferometric binaries in our sample amounts to 25%.
Balega Yuri Yu.
Dyachenko Valerii
Maksimov A. F.
Malogolovets Evgeny V.
Rastegaev D. A.
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