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Ten CoRoT eclipsing binaries: photometric solutions
(ELSEVIER, 2011)
A Close-in Substellar Object Orbiting the sdOB-type Eclipsing-Binary System NSVS14256825
(National Astronomical Observatories, 2019-09)
NSVS 14256825 is the second sdOB + dM eclipsing binary systems with anorbital period of 2.65 hours. The special binary was reported to contain circumbinary planets or brown dwarfs by using the timing method. However, ...
Eclipsing Am binary systems in the superWASP survey
(EDP Sciences, 2014-04)
The results of a search for eclipsing Am star binaries using photometry from the SuperWASP survey are presented. The light curves of 1742 Am stars fainter than V = 8.0 were analysed for the presence of eclipses. A total ...
The magnetic field and the evolution of element spots on the surface of the HgMn eclipsing binary AR Aur
(Oxford University Press, 2010-10)
The system AR Aur is a young late B-type double-lined eclipsing binary with a primary star of HgMn peculiarity. We applied the Doppler imaging method to reconstruct the distribution of Fe and Y over the surface of the ...
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 ...
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 ...