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Mount Suhora High Cadence Photometric Survey of T Tauri-Type Stars

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Języki publikacji
EN
Abstrakty
EN
Results of high-cadence multi-color observations of 121 pre-main sequence stars available from the northern hemisphere are presented. The aim of this survey was to detect transit-like signatures caused by occultation of these young stars and their accretion-induced hot spots by close-in planets and/or dusty clumps. Although none planetary transits were detected, our data allow the determination of rotational periods for some T Tau stars and characterization of the accretion processes operating in classical T Tau-type stars in time scales ranging from a few minutes to days, as well as characterization of the large-scale dips caused by dusty warped disks.
Czasopismo
Rocznik
Strony
227--260
Opis fizyczny
Bibliogr. 87 poz., rys., tab., wykr.
Twórcy
autor
  • Mount Suhora Astronomical Observatory, Cracow Pedagogical University, ul. Podchorążych 2, 30-084 Kraków, Poland
autor
  • Mount Suhora Astronomical Observatory, Cracow Pedagogical University, ul. Podchorążych 2, 30-084 Kraków, Poland
autor
  • Mount Suhora Astronomical Observatory, Cracow Pedagogical University, ul. Podchorążych 2, 30-084 Kraków, Poland
autor
  • Mount Suhora Astronomical Observatory, Cracow Pedagogical University, ul. Podchorążych 2, 30-084 Kraków, Poland
autor
  • Mount Suhora Astronomical Observatory, Cracow Pedagogical University, ul. Podchorążych 2, 30-084 Kraków, Poland
  • Mount Suhora Astronomical Observatory, Cracow Pedagogical University, ul. Podchorążych 2, 30-084 Kraków, Poland
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Uwagi
Opracowanie rekordu ze środków MNiSW, umowa Nr 461252 w ramach programu "Społeczna odpowiedzialność nauki" - moduł: Popularyzacja nauki i promocja sportu (2020)
Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-32ecff33-fd9f-4df5-bd5c-2dff8edfe848
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