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"Constant" eclipsing binary in the instability strip
DOI: 10.1016/j.newast.2014.12.006
Bibcode: 2015NewA...37...70C
Çakırlı, Ö.
The eclipsing binary OO Peg consist of two late-A type stars in circular orbit with a period of 2.985 days. I use the high-resolution spectroscopic and extensive light curves from the ASAS and Hipparcos survey to measure the physical properties of the system. Previous attempts to model the light and radial velocity curves of the system have met wi…
2015
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New Astronomy
Hipparcos
0