QIAN, Sheng-Bang, Li-Ying ZHU, Wen-Ping LIAO, Miloslav ZEJDA, Zdeněk MIKULÁŠEK, E.F. LAJUS, Staszek ZOLA, X. ZHOU and Z. HAN. Planets and Brown Dwarfs Orbiting Evolved Binaries. In Rucinski, SM Torres, G Zejda, M. LIVING TOGETHER: PLANETS, HOST STARS, AND BINARIES. SAN FRANCISCO: ASTRONOMICAL SOC PACIFIC, 2015, p. 388-393. ISBN 978-1-58381-877-0.
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Basic information
Original name Planets and Brown Dwarfs Orbiting Evolved Binaries
Name in Czech Planety a hnědí trpaslíci obíhající kole vyvinutých dvojhvězd
Authors QIAN, Sheng-Bang (156 China), Li-Ying ZHU (156 China), Wen-Ping LIAO (156 China), Miloslav ZEJDA (203 Czech Republic, guarantor, belonging to the institution), Zdeněk MIKULÁŠEK (203 Czech Republic, belonging to the institution), E.F. LAJUS (32 Argentina), Staszek ZOLA (616 Poland), X. ZHOU (156 China) and Z. HAN (156 China).
Edition SAN FRANCISCO, LIVING TOGETHER: PLANETS, HOST STARS, AND BINARIES, p. 388-393, 6 pp. 2015.
Publisher ASTRONOMICAL SOC PACIFIC
Other information
Original language English
Type of outcome Proceedings paper
Field of Study 10308 Astronomy
Country of publisher United States of America
Confidentiality degree is not subject to a state or trade secret
Publication form printed version "print"
RIV identification code RIV/00216224:14310/15:00086976
Organization unit Faculty of Science
ISBN 978-1-58381-877-0
UT WoS 000369467900092
Keywords in English ECLIPSING BINARY; CIRCUMBINARY PLANET; COMPANION; SYSTEM; STARS; VIR
Tags AKR, rivok
Tags International impact, Reviewed
Changed by Changed by: Ing. Andrea Mikešková, učo 137293. Changed: 20/4/2016 10:55.
Abstract
Searches for planets and brown dwarf companions to evolved close binary stars (e.g., detached WD+dM binaries, sdB-type eclipsing binaries, magnetic CVs, and X-ray binaries) can provide insight into the formation and ultimate fate of circumbinary planets and brown dwarfs, as well as shed light on the late evolution of binary stars. The eclipse timing method has most successfully been applied to detect extrasolar planets around binary stars evolved beyond the first red-giant branch. We have monitored different types of evolved eclipsing binaries using this method since 2006. In this paper we review some observational results of circumbinary planets and brown dwarfs orbiting evolved binaries, especially those orbiting sdB-type eclipsing binaries. The fate of the Earth in our solar system is discussed by a comparison of the observational properties of the close-in substellar objects orbiting sdB-type binaries with those of planets in our solar system.
Links
LG12001, research and development projectName: Výzkum vlastností asteroidů a hvězdných soustav pomocí fotometrických pozorování s dánským 1,54m dalekohledem (DK154) na Evropské jižní observatoři ESO (Acronym: DK154Czech)
Investor: Ministry of Education, Youth and Sports of the CR
LH14300, research and development projectName: Výzkum zvláštních proměnných hvězd
Investor: Ministry of Education, Youth and Sports of the CR
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