Detailed Information on Publication Record
2020
A photometric study of HAT 141-03513: another twin of the V361 Lyr system
WOLF, M. and Hana KUČÁKOVÁBasic information
Original name
A photometric study of HAT 141-03513: another twin of the V361 Lyr system
Authors
WOLF, M. and Hana KUČÁKOVÁ (203 Czech Republic, belonging to the institution)
Edition
NEW ASTRONOMY, 2020, 1384-1076
Other information
Language
English
Type of outcome
Článek v odborném periodiku
Field of Study
10308 Astronomy
Country of publisher
Netherlands
Confidentiality degree
není předmětem státního či obchodního tajemství
References:
RIV identification code
RIV/47813059:19630/20:A0000067
Organization unit
Institute of physics in Opava
UT WoS
000539402600017
Keywords in English
binaries: eclipsing; binaries: close; binaries: low-mass; stars: individual: HAT 141-03513; stars: individual: V361 Lyr; stars: individual: V549 Cam; stars: fundamental parameters
Tags
International impact, Reviewed
Změněno: 19/4/2021 21:45, Mgr. Pavlína Jalůvková
Abstract
V originále
The BVRI light curves were measured for the eclipsing binary HAT 141-03513 as a part of our long-term observational project for studying low-mass eclipsing binaries with a short orbital period. The asymmetric light curve and the difference in brightness in maxima, are probably the result of presence of a hot region on the surface of one component. The light curve solution in PHOEBE results to the semidetached, nearly contact configuration, where the primary fills its Roche lobe. The temperature of primary component was fixed to T-1 = 4220 K according to GAIA results, which gives us T-2 = 3555 +/- 150 K for the secondary. The spectral type of the primary component was estimated to be K6 and the photometric mass ratio was derived q = 0.435 +/- 0.015. Characteristics of the hot region were estimated. The properties of this mass-exchanging semidetached binary are compared with two previously known similar systems, V361 Lyr and V549 Cam.