Interactions between planets and evolved stars
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F16%3A00113670" target="_blank" >RIV/00216224:14310/16:00113670 - isvavai.cz</a>
Výsledek na webu
<a href="https://iopscience.iop.org/article/10.1088/1742-6596/728/4/042006" target="_blank" >https://iopscience.iop.org/article/10.1088/1742-6596/728/4/042006</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1088/1742-6596/728/4/042006" target="_blank" >10.1088/1742-6596/728/4/042006</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Interactions between planets and evolved stars
Popis výsledku v původním jazyce
Searching for planetary companions to evolved stars (e.g.,white dwarfs (WD) and Cataclysmic Variables (CV)) can provide insight into the interaction between planets and evolved stars as well as on the ultimate fate of planets. We have monitored decades of CVs and their progenitors including some detached WD binaries since 2006 to search for planets orbiting these systems. In the present paper, we will show some observational results of circumbinary planets in orbits around CVs and their progenitors. Some of our findings include planets with the shortest distance to the central evolved binaries and a few multiple planetary systems orbiting binary stars. Finally, by comparing the observational properties of planetary companions to single WDs and WD binaries, the interaction between planets and evolved stars and the ultimate fate of planets are discussed.
Název v anglickém jazyce
Interactions between planets and evolved stars
Popis výsledku anglicky
Searching for planetary companions to evolved stars (e.g.,white dwarfs (WD) and Cataclysmic Variables (CV)) can provide insight into the interaction between planets and evolved stars as well as on the ultimate fate of planets. We have monitored decades of CVs and their progenitors including some detached WD binaries since 2006 to search for planets orbiting these systems. In the present paper, we will show some observational results of circumbinary planets in orbits around CVs and their progenitors. Some of our findings include planets with the shortest distance to the central evolved binaries and a few multiple planetary systems orbiting binary stars. Finally, by comparing the observational properties of planetary companions to single WDs and WD binaries, the interaction between planets and evolved stars and the ultimate fate of planets are discussed.
Klasifikace
Druh
D - Stať ve sborníku
CEP obor
—
OECD FORD obor
10308 - Astronomy (including astrophysics,space science)
Návaznosti výsledku
Projekt
—
Návaznosti
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Ostatní
Rok uplatnění
2016
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název statě ve sborníku
11TH PACIFIC RIM CONFERENCE ON STELLAR ASTROPHYSICS: PHYSICS AND CHEMISTRY OF THE LATE STAGES OF STELLAR EVOLUTION, PTS 1-6
ISBN
—
ISSN
1742-6588
e-ISSN
—
Počet stran výsledku
8
Strana od-do
1-8
Název nakladatele
IOP PUBLISHING LTD
Místo vydání
BRISTOL
Místo konání akce
Univ Hong Kong, Hong Kong, PEOPLES R CHINA
Datum konání akce
14. 12. 2015
Typ akce podle státní příslušnosti
WRD - Celosvětová akce
Kód UT WoS článku
000397958000031