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Cluster AgeS Experiment (CASE): Dwarf Novae and a Probable Microlensing Event in the Globular Cluster M22

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Języki publikacji
EN
Abstrakty
EN
We report the identification of a new cataclysmic variable (denoted as CV2) and a probable microlensing event in the field of the globular cluster M22. Two outbursts were observed for CV2. During one of them superhumps with Psh=0.08875 d were present in the light curve. CV2 has an X-ray counterpart detected by XMM-Newton. A very likely microlensing event at a radius of 2.'3 from the cluster center was detected. It had an amplitude of Δ V=0.75 mag and a characteristic time of 15.9 days. Based on model considerations we show that the most likely configuration has the source in the Galactic bulge with the lens in the cluster. Two outbursts were observed for the already known dwarf nova CV1.
Czasopismo
Rocznik
Strony
261--274
Opis fizyczny
Bibliogr. 39 poz., rys., tab., wykr.
Twórcy
  • Nicolaus Copernicus Astronomical Center, ul. Bartycka 18, 00-716 Warsaw, Poland
autor
  • Nicolaus Copernicus Astronomical Center, ul. Bartycka 18, 00-716 Warsaw, Poland
  • arnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, CA 91101, USA
  • Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warsaw, Poland
  • Nicolaus Copernicus Astronomical Center, ul. Bartycka 18, 00-716 Warsaw, Poland
  • Astronomical Observatory, Adam Mickiewicz University, ul. Słoneczna 36, 61-286 Poznań, Poland
  • Las Campanas Observatory, Casilla 601, La Serena, Chile
autor
  • Nicolaus Copernicus Astronomical Center, ul. Bartycka 18, 00-716 Warsaw, Poland
Bibliografia
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Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-81e839cb-55e3-4f36-aea4-40b582d222b6
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