D 2015

Planets and Brown Dwarfs Orbiting Evolved Binaries

QIAN, Sheng-Bang, Li-Ying ZHU, Wen-Ping LIAO, Miloslav ZEJDA, Zdeněk MIKULÁŠEK et. al.

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

Language

English

Type of outcome

Stať ve sborníku

Field of Study

10308 Astronomy

Country of publisher

United States of America

Confidentiality degree

není předmětem státního či obchodního tajemství

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

Tags

International impact, Reviewed
Změněno: 20/4/2016 10:55, Ing. Andrea Mikešková

Abstract

V originále

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 project
Name: 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 project
Name: Výzkum zvláštních proměnných hvězd
Investor: Ministry of Education, Youth and Sports of the CR