Detailed Information on Publication Record
2016
Time-dependent spectral-feature variations of stars displaying the B[e] phenomenon III. HD 50138
JEŘÁBKOVÁ, Tereza, Daniela KORČÁKOVÁ, A. MIROSHNICHENKO, S. DANFORD, S.V. ZHARIKOV et. al.Basic information
Original name
Time-dependent spectral-feature variations of stars displaying the B[e] phenomenon III. HD 50138
Authors
JEŘÁBKOVÁ, Tereza (203 Czech Republic), Daniela KORČÁKOVÁ (203 Czech Republic), A. MIROSHNICHENKO (643 Russian Federation), S. DANFORD (840 United States of America), S.V. ZHARIKOV (643 Russian Federation), Radek KŘÍČEK (203 Czech Republic), Petr ZASCHE (203 Czech Republic), Viktor VOTRUBA (203 Czech Republic, belonging to the institution), Miroslav ŠLECHTA (203 Czech Republic), Petr ŠKODA (203 Czech Republic) and Jan JANÍK (203 Czech Republic, guarantor, belonging to the institution)
Edition
Astronomy and Astrophysics, EDP Sciences, 2016, 0004-6361
Other information
Language
English
Type of outcome
Článek v odborném periodiku
Field of Study
10308 Astronomy
Country of publisher
France
Confidentiality degree
není předmětem státního či obchodního tajemství
Impact factor
Impact factor: 4.378 in 2014
RIV identification code
RIV/00216224:14310/16:00089235
Organization unit
Faculty of Science
UT WoS
000369715900127
Keywords in English
circumstellar matter; stars: emission line Be; stars: mass loss; binaries: spectroscopic; stars: individual: MWC 158
Tags
International impact, Reviewed
Změněno: 3/4/2019 14:13, RNDr. Jan Janík, Ph.D.
Abstract
V originále
We describe the spectral variability of HD 50138 over the last twenty years. Based on these data, we determine new restrictions for future modelling. We confirm the quasi-periodic behaviour of the object’s spectral variability, which probably reflects mass transfer in a binary system. This behaviour also supports a recently introduced explanation of the nature of FS CMa stars as post-merger systems.