OSU Navigation Bar

The Ohio State University University Libraries Knowledge Bank

The Knowledge Bank is scheduled for regular maintenance on Sunday, April 20th, 8:00 am to 12:00 pm EDT. During this time users will not be able to register, login, or submit content.

The Lowest Mass White Dwarf

Please use this identifier to cite or link to this item: http://hdl.handle.net/1811/48213

Show full item record

Files Size Format View
fac_KilicM_TheA ... lJournal_2007_660_1451.pdf 952.4Kb PDF View/Open

Title: The Lowest Mass White Dwarf
Creators: Kilic, Mukremin; Prieto, Carlos Allende; Brown, Warren R.; Koester, D.
Keywords: white dwarfs
stars: low-mass, brown dwarfs
Issue Date: 2007-05-10
Publisher: American Astronomical Society
Citation: Mukremin Kilic et al, "The Lowest Mass White Dwarf," The Astrophysical Journal 660, no. 2 (2007), doi:10.1086/514327
DOI: 10.1086/514327
Abstract: Extremely low mass white dwarfs are very rare objects likely formed in compact binary systems. We present MMT optical spectroscopy of 42 low-mass white dwarf candidates serendipitously discovered in a survey for hypervelocity B-type stars. One of these objects, SDSS J0917+46, has T_eff = 11,288 ± 72 K and log g = 5.48 ± 0.03; with an estimated mass of 0.17 Msun, it is the lowest gravity/mass white dwarf currently known. However, 40 of the low-mass candidates are normal DA white dwarfs with apparently inaccurate SDSS g magnitudes. We revisit the identification of low-mass white dwarf candidates previously found in the SDSS and conclude that four objects have M < 0.2 Msun. None of these white dwarfs show excess emission from a binary companion, and radial velocity searches will be necessary to constrain the nature of the unseen companions.
ISSN: 1538-4357
URI: http://hdl.handle.net/1811/48213
Bookmark and Share