A New Gravitational Wave Verification Source
Mukremin Kilic, Warren R. Brown, A. Gianninas, J. J. Hermes, Carlos, Allende Prieto, S. J. Kenyon

TL;DR
This paper reports the discovery of a short-period binary white dwarf system, WD0931+444, which is a promising gravitational wave verification source detectable by space-based observatories like eLISA.
Contribution
It identifies WD0931+444 as the second-shortest period detached binary white dwarf system and confirms its potential as a gravitational wave verification source.
Findings
WD0931+444 has a 20-minute orbital period.
The system will merge in less than 9 million years.
It is a confirmed gravitational wave verification source for eLISA.
Abstract
We report the discovery of a detached 20 min orbital period binary white dwarf. WD0931+444 (SDSS J093506.93+441106.9) was previously classified as a WD + M dwarf system based on its optical spectrum. Our time-resolved optical spectroscopy observations obtained at the 8m Gemini and 6.5m MMT reveal peak-to-peak radial velocity variations of 400 km/s every 20 min for the WD, but no velocity variations for the M dwarf. In addition, high-speed photometry from the McDonald 2.1m telescope shows no evidence of variability nor evidence of a reflection effect. An M dwarf companion is physically too large to fit into a 20 min orbit. Thus, the orbital motion of the WD is almost certainly due to an invisible WD companion. The M dwarf must be either an unrelated background object or the tertiary component of a hiearchical triple system. WD0931+444 contains a pair of WDs, a 0.32 Msol primary and a…
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