The catalogue of stellar parameters from the detached double-lined eclipsing binaries in the milky way

64Citations
Citations of this article
15Readers
Mendeley users who have this article in their library.

Abstract

The most accurate stellar astrophysical parameters were collected from the solutions of the light and the radial velocity curves of 257 detached double-lined eclipsing binaries in the Milky Way. The catalogue contains masses, radii, surface gravities, effective temperatures, luminosities, projected rotational velocities of the component stars, and the orbital parameters. The number of stars with accurate parameters increased 67% in comparison to the most recent similar collection by Torres, Andersen, & Giménez (2010). Distributions of some basic parameters were investigated. The ranges of effective temperatures, masses, and radii are 2750 < 43000, 0.18 < 33, and 0.2 < 21.2, respectively. Being mostly located in one kpc in the Solar neighborhood, the present sample covers distances up to 4.6 kpc within the two local Galactic arms, Carina-Sagittarius and Orion Spur. The number of stars with both mass and radius measurements better than 1% uncertainty is 93, better than 3% uncertainty is 311, and better than 5% uncertainty is 388. It is estimated from the Roche lobe filling factors that 455 stars (88.5% of the sample) are spherical within 1% of uncertainty. © 2014 Astronomical Society of Australia.

Cite

CITATION STYLE

APA

Eker, Z., Bilir, S., Soydugan, F., Gökçe, E. Y., Soydugan, E., Tüysüz, M., … Demircan, O. (2014). The catalogue of stellar parameters from the detached double-lined eclipsing binaries in the milky way. Publications of the Astronomical Society of Australia, 31(1). https://doi.org/10.1017/pasa.2014.17

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free