Tytuł artykułu
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Wybrane pełne teksty z tego czasopisma
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Warianty tytułu
Języki publikacji
Abstrakty
The loneliness of hot Jupiters supports the high-eccentricity migration as a primary path leading to the formation of systems with those planets stripped of any close-in planetary companions. Here we present the null results of searches for low-mass planets close to hot Jupiters in 10 planetary systems: HAT-P-4, HAT-P-10, HAT-P-12, HAT-P-17, HAT-P-19, HAT-P-32, HAT-P-44, Qatar-6, TrES-4, and WASP-48. We employed multi-sector time-series photometry from the Transiting Exoplanet Survey Satellite enhanced with new ground-based transit light curves to determine the sizes of hypothetical planets that might still avoid being detected. We redetermined transit parameters for the known hot Jupiters using a homogeneous approach. We refuted transit timing variations for HAT-P-12 b, claimed recently in the literature. The transit timing data permitted us to place tighter constraints on third bodies in HAT-P-19 and HAT-P-32 systems detected in Doppler measurements. We also study four multi-periodic pulsating variable stars in the field around HAT-P-17.
Słowa kluczowe
planetary systems
stars: individual: HAT-P-4
stars: individual: HAT-P-10
stars: individual: HAT-P-12
stars: individual: HAT-P-17
stars: individual: HAT-P-19
stars: individual: HAT-P-32
stars: individual: HAT-P-44
stars: individual: Qatar-6
stars: individual: TrES-4
stars: individual: WASP-48
stars: individual: BD+30 4487
stars: individual: TYC 2717-453-1
stars: individual: Gaia DR3 11849720750852486656
stars: individual: Gaia DR3 1849743737517511296
planets and satellites: individual: HAT-P-4 b
planets and satellites: individual: HAT-P-10 b
planets and satellites: individual: HAT-P-12
planets and satellites: individual: HAT-P-17 b
planets and satellites: individual: HAT-P-19 b
planets and satellites: individual: HAT-P-32 b
planets and satellites: individual: HAT-P-44 b
planets and satellites: individual: Qatar-6 b
planets and satellites: individual: TrES-4 b
planets and satellites: individual: WASP-48 b
Czasopismo
Rocznik
Tom
Strony
57--86
Opis fizyczny
Bibliogr. 97 poz., tab., wykr.
Twórcy
autor
- Institute of Astronomy, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toruń, Grudziądzka 5, 87-100 Toruń, Poland
autor
- Instituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía 3, 18008 Granada, Spain
autor
- Instituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía 3, 18008 Granada, Spain
autor
- Instituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía 3, 18008 Granada, Spain
autor
- Michael Adrian Observatorium, Astronomie Stiftung Trebur, 65428 Trebur, Germany
- University of Applied Sciences, Technische Hochschule Mittelhessen, 61169 Friedberg, Germany
autor
- Astrophysikalisches Institut und Universitäts-Sternwarte, Schillergäßchen 2, 07745 Jena, Germany
autor
- Astrophysikalisches Institut und Universitäts-Sternwarte, Schillergäßchen 2, 07745 Jena, Germany
autor
- Astrophysikalisches Institut und Universitäts-Sternwarte, Schillergäßchen 2, 07745 Jena, Germany
autor
- Astrophysikalisches Institut und Universitäts-Sternwarte, Schillergäßchen 2, 07745 Jena, Germany
autor
- Institute of Astronomy, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toruń, Grudziądzka 5, 87-100 Toruń, Poland
autor
- Valencia International University, 46002 Valencia, Spain
autor
- Valencia International University, 46002 Valencia, Spain
autor
- Valencia International University, 46002 Valencia, Spain
autor
- Valencia International University, 46002 Valencia, Spain
autor
- Valencia International University, 46002 Valencia, Spain
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Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-6b40744a-31dc-49cd-bd3e-f878795a85fc