Super-Fast Line-Profile Variability in the Spectra of OBA-Stars: B1-Star ρ Leo


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This study continues our investigation of the super-fast variability of line profiles in the spectra of early-type stars. We have investigated the line-profile variability in spectra of OBA-stars with the SCORPIO multi-mode focal reducer mounted at the 6-m SAO RAS telescope. Regular short-period variations of the H and He lines in the spectra of the B1I star ρ Leo were detected with periods ranging from 2 to 90 minutes, as well as irregular line-profile variations on time intervals less than 1 minute. A possible origin of rapid spectral variations is discussed.

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A. Kholtygin

St. Petersburg State University

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Email: afkholtygin@gmail.com
俄罗斯联邦, St. Petersburg, 198504

A. Batrakov

St. Petersburg State University

Email: afkholtygin@gmail.com
俄罗斯联邦, St. Petersburg, 198504

S. Fabrika

Special Astrophysical Observatory

Email: afkholtygin@gmail.com
俄罗斯联邦, Nizhnii Arkhyz, 369167

A. Valeev

Special Astrophysical Observatory

Email: afkholtygin@gmail.com
俄罗斯联邦, Nizhnii Arkhyz, 369167

I. Tumanova

St. Petersburg State University

Email: afkholtygin@gmail.com
俄罗斯联邦, St. Petersburg, 198504

O. Tsiopa

Pulkovo astronomical observatory of the Russian Academy of Sciences

Email: afkholtygin@gmail.com
俄罗斯联邦, St. Petersburg, 196140

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