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A Low-Resolution Spectroscopic Exploration of Puzzling OGLE Variable Stars

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Języki publikacji
EN
Abstrakty
EN
We present the results of a spectroscopic follow-up of various puzzling variable objects detected in the OGLE-III Galactic disk and bulge fields. The sample includes mainly short-period multi-mode pulsating stars that could not have been unambiguously classified as either δ Sct or β Cep type stars based on photometric data only, also stars with irregular fluctuations mimicking cataclysmic variables and stars with dusty shells, and periodic variables displaying brightenings in their light curves that last for more than half of the period. The obtained low-resolution spectra show that all observed short-period pulsators are of δ Sct type, the stars with irregular fluctuations are young stellar objects, and the objects with regular brightenings are A type stars or very likely Ap stars with strong magnetic field responsible for the presence of bright caps around magnetic poles on their surface. We also took spectra of objects designated OGLE-GD-DSCT-0058 and OGLE-GD-CEP-0013. An estimated effective temperature of 33 000 K in OGLE-GD-DSCT-0058 indicates that it cannot be a δ Sct type variable. This very short-period (0.01962 d) high-amplitude (0.24 mag in the I-band) object remains a mystery. It may represent a new class of variable stars. The spectrum of OGLE-GD-CEP-0013 confirms that this is a classical Cepheid despite a peculiar shape of its light curve. The presented results will help in proper classification of variable objects in the OGLE Galaxy Variability Survey.
Czasopismo
Rocznik
Strony
63--79
Opis fizyczny
Bibliogr. 33 poz., tab., wykr.
Twórcy
  • Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
autor
  • Dr. Karl Remeis-Observatory & ECAP, Astronomical Institute, Friedrich-Alexander University Erlangen-Nuremberg, Sternwartstrasse 7, D-96049 Bamberg, Germany
autor
  • Gemini Observatory, Casilla 603, La Serena, Chile
autor
  • Las Campanas Observatory, Casilla 601, La Serena, Chile
  • Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
autor
  • Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
autor
  • Departamento de Fisica, Universidade Federal do Maranhão, São Luis, MA, Brazil
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Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-0cb87ec9-58fc-4b2b-b935-3c85611f7234
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