Photoelectric radial velocities of eclipsing binaries. IV - BW Aqr: Spectroscopic orbit, masses, and radii

Astronomy and Astrophysics – Astrophysics

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Eclipsing Binary Stars, Orbital Elements, Radial Velocity, Stellar Mass, Stellar Orbits, Stellar Spectrophotometry, Dwarf Stars, Electrophotometry, Radii

Scientific paper

Spectroscopic and photoelectric radial velocities of the 10th magnitude double-lined eclipsing binary BW Aqr are presented and discussed in conjonction with the recent photometric data by Khaliullin and Kozureva. The orbital elements have been determined from 14 double-lined spectra and 25 accurate photoelectric radial velocity determinations. We derive orbital elements: V0=9.9 km s-1, KA=78.4 km s-1, KB=84.2 km s-1, e=0.178. The combination of these elements with the relative orbit from photometric data leads us to adopt for the system MA=1.48 Msun, MB = 1.38 Msun, RA= 2.08 Rsun , RB = 1.81 Rsun and a = 21.3 Rsun.

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