The ELM Survey. II. Twelve Binary White Dwarf Merger Systems

Kilic, Mukremin; Brown, Warren R.; Allende-Prieto, C.; Agüeros, M. A.; Heinke, Craig; Kenyon, S. J.
Bibliographical reference

The Astrophysical Journal, Volume 727, Issue 1, article id. 3 (2011).

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1
2011
Number of authors
6
IAC number of authors
1
Citations
122
Refereed citations
105
Description
We describe new radial velocity and X-ray observations of extremely low-mass white dwarfs (ELM WDs, ~0.2 M sun) in the Sloan Digital Sky Survey Data Release 4 and the MMT Hypervelocity Star survey. We identify four new short period binaries, including two merger systems. These observations bring the total number of short period binary systems identified in our survey to 20. No main-sequence or neutron star companions are visible in the available optical photometry, radio, and X-ray data. Thus, the companions are most likely WDs. Twelve of these systems will merge within a Hubble time due to gravitational wave radiation. We have now tripled the number of known merging WD systems. We discuss the characteristics of this merger sample and potential links to underluminous supernovae, extreme helium stars, AM CVn systems, and other merger products. We provide new observational tests of the WD mass-period distribution and cooling models for ELM WDs. We also find evidence for a new formation channel for single low-mass WDs through binary mergers of two lower mass objects. Based on observations obtained at the MMT Observatory, a joint facility of the Smithsonian Institution and the University of Arizona.
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