1. Primeval very low-mass stars and brown dwarfs – VIII. The first age benchmark L subdwarf, a wide companion to a halo white dwarf.
- Author
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(张曾华), Z H Zhang, Raddi, R, Burgasser, A J, Casewell, S L, Smart, R L, Gálvez-Ortiz, M C, Jones, H R A, Baig, S, Lodieu, N, Gauza, B, Pavlenko, Ya V, (焦云帆), Y F Jiao, (赵坤瑶), Z K Zhao, (周思琰), S Y Zhou, and Pinfield, D J
- Subjects
BROWN dwarf stars ,STELLAR populations ,DWARF stars ,LOW mass stars ,GALACTIC halos ,WHITE dwarf stars - 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. [ABSTRACT FROM AUTHOR]- Published
- 2024
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