Research output: Chapter in Book/Report/Conference proceeding › Conference contribution
Short Timescale Line Profile Variations in Spectra of OB Stars: the Case of ρ Leo. / Batrakov, A.A.; Kholtygin, A.F.; Fabrika, S.; Valeev, A.
Physics of Magnetic Stars: Proceedings of a Conference Held at Special Astrophysical Observatory, Nizhny Arkhyz, Russia, 1-5 October 2018. ed. / I.I. Romanyuk; I. A. Yakunin; D.O. Kudryavtsev. San Francisco : Astronomical Society of the Pacific, 2019. p. 151-153 (Astronomical Society of the Pacific Conference Series; Vol. 518).Research output: Chapter in Book/Report/Conference proceeding › Conference contribution
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TY - GEN
T1 - Short Timescale Line Profile Variations in Spectra of OB Stars: the Case of ρ Leo
AU - Batrakov, A.A.
AU - Kholtygin, A.F.
AU - Fabrika, S.
AU - Valeev, A.
PY - 2019/7/1
Y1 - 2019/7/1
N2 - The paper continues the study of superfast line profile variations (LPV) in spectra of early-type stars. The multimode focal reducer SCORPIO at the 6-meter telescope (BTA) was used to obtain 1271 low-resolution spectra of ρ Leo (B1 Iab). Regular LPVs for H I, He I, Fe II, N II, O II, Si III, and other ion lines with periods from ̃ 2 to ̃ 90 minutes and an amplitude of 1-2% of the continuum level are detected. Nonregular LPVs were also detected at time intervals less then a minute. The harmonics of LPVs with periods less than 10 minutes appear to be variable. During 128 minutes of observation their periods can change by ̃ 40%. Possible causes of such fast spectral variations are discussed.
AB - The paper continues the study of superfast line profile variations (LPV) in spectra of early-type stars. The multimode focal reducer SCORPIO at the 6-meter telescope (BTA) was used to obtain 1271 low-resolution spectra of ρ Leo (B1 Iab). Regular LPVs for H I, He I, Fe II, N II, O II, Si III, and other ion lines with periods from ̃ 2 to ̃ 90 minutes and an amplitude of 1-2% of the continuum level are detected. Nonregular LPVs were also detected at time intervals less then a minute. The harmonics of LPVs with periods less than 10 minutes appear to be variable. During 128 minutes of observation their periods can change by ̃ 40%. Possible causes of such fast spectral variations are discussed.
M3 - Conference contribution
SN - 9781583819234
T3 - Astronomical Society of the Pacific Conference Series
SP - 151
EP - 153
BT - Physics of Magnetic Stars
A2 - Romanyuk, I.I.
A2 - Yakunin, I. A.
A2 - Kudryavtsev, D.O.
PB - Astronomical Society of the Pacific
CY - San Francisco
T2 - International Conference "Physics of Magnetic Stars"
Y2 - 1 October 2019 through 5 October 2019
ER -
ID: 49301276