Twins: The two shortest period non-interacting double degenerate white dwarf stars

F. Mullally, Carles Badenes, Susan E. Thompson, Robert Lupton

Research output: Contribution to journalArticlepeer-review

37 Scopus citations

Abstract

We report on the detection of the two shortest period non-interacting white dwarf binary systems. These systems, SDSS J143633.29+501026.8 and SDSS J105353.89+520031.0, were identified by searching for radial velocity variations in the individual exposures that make up the published spectra from the Sloan Digital Sky Survey. We followed up these systems with time series spectroscopy to measure the period and mass ratios of these systems. Although we only place a lower bound on the companion masses, we argue that they must also be white dwarf stars. With periods of approximately 1 hr, we estimate that the systems will merge in less than 100 Myr, but the merger product will likely not be massive enough to result in a Type 1a supernova.

Original languageEnglish (US)
Pages (from-to)L51-L55
JournalAstrophysical Journal
Volume707
Issue number1 PART 2
DOIs
StatePublished - 2009

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • Binaries: close
  • Binaries: spectroscopic
  • White dwarfs

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