Speckle interferometry of magnetic stars with the BTA. I. First results |
| |
| Authors: | Yu Yu Balega V V Dyachenko A F Maksimov E V Malogolovets D A Rastegaev I I Romanyuk |
| |
| Institution: | 1.Special Astrophysical Observatory,Russian Academy of Sciences,Nizhnii Arkhyz,Russia |
| |
| Abstract: | 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%. |
| |
| Keywords: | |
| 本文献已被 SpringerLink 等数据库收录！ |
|
