Warianty tytułu
Języki publikacji
Abstrakty
We present the list of variable stars we found in the Kepler superstamp data covering approximately nine arcminutes from the central region of NGC 6819. This is a continuation of our earlier work. We classified the variable stars based on the variability type and we established their cluster membership based on the available Gaia Data Release 3 astrometry. Our search revealed 385 variable stars but only 128 were found to be cluster members. In the case of eclipsing and contact binaries we calculated the mid-times of eclipses and derived ephemerides. We searched for eclipse timing variation using the observed minus calculated diagrams. Only five objects show significant orbital period variation. We used isochrones calculated within the MESA Isochrones and Stellar Tracks project and derived the average age (2.54 Gyr), average distance (2.3 kpc) and iron content [Fe/H]=-0.01(2), of NGC 6819. We confirm this distance by the one derived from Gaia astrometry of the cluster members with membership probabilities greater than 0.9.
Czasopismo
Rocznik
Tom
Strony
267--295
Opis fizyczny
Bibliogr. 63 poz., tab., wykr.
Twórcy
autor
- ARDASTELLA Research Group
- Centrum Astronomiczne im. Mikołaja Kopernika, Polskiej Akademii Nauk, ul. Bartycka 18, 00-716 Warszawa, Poland
autor
- ARDASTELLA Research Group
- Astronomical Observatory, University of Warsaw, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
autor
- ARDASTELLA Research Group
- Astroserver.org, Fötér 1, 8533 Malomsok, Hungary
- Astronomical Institute of the Czech Academy of Sciences, Fričova 298, CZ-251~65 Ondřejov, Czech Republic
autor
- Department of Astronomy, New Mexico State University, Box 30001, MSC 4500, Las Cruces, NM 88003, USA
- Apache Point Observatory, 2001 Apache Point Road, P.O. Box 59, Sunspot, NM 88349-0059
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Typ dokumentu
Bibliografia
Identyfikatory
Identyfikator YADDA
bwmeta1.element.baztech-0a04c2bc-a160-4138-9123-5675bd8bb8e0