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Fundamental parameters of the massive eclipsing binary HM1 8
(Wiley Blackwell Publishing, Inc, 2021-09)
We present a comprehensive study of the massive binary system HM1 8, based on multi-epoch high-resolution spectroscopy, V-band photometry, and archival X-ray data. Spectra from the OWN Survey, a high-resolution optical ...
Eclipsing binary stars in the era of massive surveys first results and future prospects
(2017)
Our thinking about eclipsing binary stars has undergone a tremendous change in the last decade. Eclipsing binary stars are one of nature's best laboratories for determining the fundamental physical properties of stars and ...
Fundamental parameters of the eclipsing binary DD CMa and evidence for mass exchange
(IOP Publishing, 2021-04)
We present a detailed photometric and spectroscopic analysis of DD CMa, based on published survey photometry and new spectroscopic data. We find an improved orbital period of Po = 2.0084530(6) days. Our spectra reveal Hβ ...
Binária EclipsanteEclipsing Binary
(Michael R. Gallis, 2016)
Binária EclipsanteEclipsing Binary
(Michael R. Gallis, 2011)
The Araucaria Project. Determination of the Large Magellanic Cloud Distance from Late-Type Eclipsing Binary Systems. I. OGLE-051019.64-685812.3
(2009)
We have analyzed the double-lined eclipsing binary system OGLE-051019.64-685812.3 in the LMC which consists of two G4 giant components with very similar effective temperatures. A detailed analysis of the Optical Gravitational ...
Short term period variable stars observed at OAUNI
(Universidad Nacional de Ingeniería, 2019-06-06)
We present the first scientific results of the program on short term period variable stars observed at OAUNI at the peruvian Andes. These results include good quality light curves of delta Scuti stars, rapidly oscillating ...