UBVRc Ic analysis of the recently discovered totally eclipsing extreme mass ratio binary V1853 Orionis, and a statistical look at 25 other extreme mass ratio solar-type contact binaries Article

Samec, RG, Labadorf, CM, Hawkins, NC et al. (2011). UBVRc Ic analysis of the recently discovered totally eclipsing extreme mass ratio binary V1853 Orionis, and a statistical look at 25 other extreme mass ratio solar-type contact binaries . ASTRONOMICAL JOURNAL, 142(4), 10.1088/0004-6256/142/4/117

cited authors

  • Samec, RG; Labadorf, CM; Hawkins, NC; Faulkner, DR; Van Hamme, W

authors

abstract

  • We present precision CCD light curves, a period study, photometrically derived standard magnitudes, and a five-color simultaneous Wilson code solution of the totally eclipsing, yet shallow amplitude (Av 0.4mag) eclipsing, binary V1853 Orionis. It is determined to be an extreme mass ratio, q = 0.20, W-type W UMa overcontact binary. From our standard star observations, we find that the variable is a late-type F spectral-type dwarf, with a secondary component of about 0.24 solar masses (stellar type M5V). Its long eclipse duration (41 minutes) as compared to its period, 0.383 days, attests to the small relative size of the secondary. Furthermore, it has reached a Roche lobe fill-out of 50% of its outer critical lobe as it approaches its final stages of binary star evolution, that of a fast spinning single star. Finally, a summary of about 25 extreme mass ratio solar-type binaries is given. © 2011 The American Astronomical Society. All rights reserved.

publication date

  • October 1, 2011

published in

Digital Object Identifier (DOI)

volume

  • 142

issue

  • 4