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Title: Primeval very low-mass stars and brown dwarfs – VIII. The first age benchmark L subdwarf, a wide companion to a halo white dwarf

Journal Article · · Monthly Notices of the Royal Astronomical Society

ABSTRACT We report the discovery of five white dwarf + ultracool dwarf systems identified as common proper motion wide binaries in the Gaia Catalogue of Nearby Stars. The discoveries include a white dwarf + L subdwarf binary, VVV 1256−62AB, a gravitationally bound system located 75.6$$^{+1.9}_{-1.8}$$ pc away with a projected separation of 1375$$^{+35}_{-33}$$ au. The primary is a cool DC white dwarf with a hydrogen dominated atmosphere, and has a total age of $$10.5^{+3.3}_{-2.1}$$ Gyr, based on white dwarf model fitting. The secondary is an L subdwarf with a metallicity of [M/H] = $$-0.72^{+0.08}_{-0.10}$$ (i.e. [Fe/H] = $$-0.81\pm 0.10$$) and $$T_{\rm eff}$$ = 2298$$^{+45}_{-43}$$ K based on atmospheric model fitting of its optical to near infrared spectrum, and likely has a mass just above the stellar/substellar boundary. The subsolar metallicity of the L subdwarf and the system’s total space velocity of 406 km s−1 indicates membership in the Galactic halo, and it has a flat eccentric Galactic orbit passing within 1 kpc of the centre of the Milky Way every $$\sim$$0.4 Gyr and extending to 15–31 kpc at apogal. VVV 1256−62B is the first L subdwarf to have a well-constrained age, making it an ideal benchmark of metal-poor ultracool dwarf atmospheres and evolution.

Sponsoring Organization:
USDOE
OSTI ID:
2437797
Journal Information:
Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Journal Issue: 2 Vol. 533; ISSN 0035-8711
Publisher:
Oxford University PressCopyright Statement
Country of Publication:
United Kingdom
Language:
English

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