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The Discovery of a Companion to the Lowest Mass White Dwarf*

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Mukremin Kilic1, Warren R. Brown2, Carlos Allende Prieto3, M. H. Pinsonneault1 and S. J. Kenyon2

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We report the detection of a radial velocity companion to SDSS J091709.55+463821.8, the lowest mass white dwarf currently known, with M ~ 0.17 Msun. The radial velocity of the white dwarf shows variations with a semi-amplitude of 148.8 ± 6.9 km s-1 and a period of 7.5936 ± 0.0024 hr, which implies a companion mass of M ≥ 0.28 Msun. The lack of evidence of a companion in the optical photometry forces any main-sequence companion to be smaller than 0.1 Msun, hence a low-mass main-sequence star companion is ruled out for this system. The companion is most likely another white dwarf, and we present tentative evidence for an evolutionary scenario that could have produced it. However, a neutron star companion cannot be ruled out, and follow-up radio observations are required to search for a pulsar companion.


Footnote
*  Observations reported here were obtained at the MMT Observatory, a joint facility of the Smithsonian Institution and the University of Arizona.
Subject headings

stars: individual (SDSS J091709.55+463821.8); stars: low-mass, brown dwarfs; white dwarfs


Dates

Issue 2 (2007 August 1)

Received 2007 April 3, accepted for publication 2007 April 8



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