期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 471, 期 2, 页码 1543-1552出版社
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stx1654
关键词
stars: abundances; stars: evolution; stars: individual: CPD-57 degrees 3509; stars: magnetic field; stars: massive; stars: oscillations
资金
- ESO Telescopes at the La Silla Paranal Observatory [094.D-0355, 191.D-0255]
- Nordrhein-Westfalische Akademie der Wissenschaften und der Kunste
- RFBR [16-02-00604A]
The magnetic field of CPD -57 degrees 3509 was recently detected in the framework of the BOB (B fields in OB stars) collaboration. We acquired low-resolution spectropolarimetric observations of CPD -57 degrees 3509 with the FOcal Reducer low-dispersion Spectrograph 2 and high-resolution UV-Visual Echelle Spectrograph observations randomly distributed over a few months to search for periodicity, to study the magnetic field geometry and to determine the surface distribution of silicon and helium. We also obtained supplementary photometric observations at a timeline similar to the spectroscopic and spectropolarimetric observations. A period of 6.36 d was detected in the measurements of the mean longitudinal magnetic field. A sinusoidal fit to our measurements allowed us to constrain the magnetic field geometry and estimate the dipole strength in the range of 3.9-4.5 kG. Our application of the Doppler imaging technique revealed the presence of He I spots located around the magnetic poles, with a strong concentration at the positive pole and a weaker one around the negative pole. In contrast, high-concentration Si III spots are located close to the magnetic equator. Furthermore, our analysis of the spectral variability of CPD -57 degrees 3509 on short time-scales indicates distinct changes in shape and position of line profiles possibly caused by the presence of beta Cep like pulsations. A small periodic variability in line with the changes of the magnetic field strength is clearly seen in the photometric data.
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