LP 133-373: A New Chromospherically Active Eclipsing dMe Binary with a Distant, Cool White Dwarf Companion

Todd R. Vaccaro, A. Kawka, T. D. Oswalt, I. Silver, M. Wood, J. Allyn Smith

Research output: Contribution to journalArticlepeer-review

Abstract

We report the discovery of the partially eclipsing binary LP 133-373. Nearly identical eclipses along with observed photometric colors and spectroscopy indicate that it is a pair of chromospherically active dM4 stars in a circular 1.6 day orbit. Light and velocity curve modeling to our differential photometry and velocity data show that each star has a mass and radius of 0.340+/-0.014 M solar and 0.33+/-0.02 R solar . The binary is itself part of a common proper motion pair with LP 133-374, a cool DC or possible DA white dwarf with a mass of 0.49-0.82 M solar , which would make the system at least 3 Gyr old

Original languageAmerican English
JournalAstrophysical Journal
StatePublished - Jun 1 2007
Externally publishedYes

Keywords

  • binaries: eclipsing
  • stars: activity
  • white dwarfs

Disciplines

  • Astrophysics and Astronomy
  • Stars, Interstellar Medium and the Galaxy

Cite this