10 citations · 26 across the 5 of their papers we have counts for
8 papers
A search for the presence of magnetic fields in the two Supergiant Fast X-ray Transients IGR J08408-4503 and IGR J11215-5952
S. Hubrig, L. Sidoli, K. Postnov +4
A significant fraction of high-mass X-ray binaries are supergiant fast X-ray transients (SFXTs). The prime model for the physics governing their X-ray behaviour suggests that the w…
Magnetic field and radial velocities of the star Chi Draconis A
Byeong-Cheol Lee, D. Gadelshin, Inwoo Han +13
We present high-resolution spectropolarimetric observations of the spectroscopic binary Chi Dra. Spectral lines in the spectrum of the main component Chi Dra A show variable Zeeman…
Statistics of magnetic field measurements and evolution of magnetic field of OBA stars
A. S. Medvedev, A. F. Kholtygin, S. Hubrig +7
We review the measurements of magnetic fields of OBA stars. Based on these data we confirm that magnetic fields are distributed according to a lognormal law with a mean log(B)=-0.5…
Magnetic field geometry and chemical abundance distribution of the He-strong star CPD -57 3509
S. Hubrig, N. Przybilla, H. Korhonen +9
The magnetic field of CPD -57 3509 was recently detected in the framework of the BOB (B fields in OB stars) collaboration. We acquired low-resolution spectropolarimetric observatio…
The first spectropolarimetric monitoring of the peculiar O4Ief supergiant zeta Puppis
S. Hubrig, A. Kholtygin, I. Ilyin +2
The origin of the magnetic field in massive O-type stars is still under debate. To model the physical processes responsible for the generation of O star magnetic fields, it is impo…
Smoothed Temporal Variance Spectrum: weak line profile variations and NRP diagnostics
A. F. Kholtygin, N. P. Sudnik
We describe the version of the Temporal Variance Spectrum (TVS, Fullerton, Gies & Bolton 1996) method with pre-smoothed line profile (smoothed Temporal Variance Spectrum, smTVS). T…