Primeval very low-mass stars and brown dwarfs: IV. New L subdwarfs, Gaia astrometry, population properties, and a blue brown dwarf binary
ABSTRACT. We present 27 new L subdwarfs and classify five of them as esdL and 22 as sdL. Our L subdwarf candidates were selected with the UKIRT Infrared Deep S
Gespeichert in:
| Hauptverfasser: | , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2018 July 31
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 480, Heft: 4, Pages: 5447-5474 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty2054 |
| Online-Zugang: | Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty2054 Verlag, Volltext: https://academic.oup.com/mnras/article/480/4/5447/5062823 
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| Verfasserangaben: | Z.H. Zhang (张曾华), M.C. Galvez-Ortiz, D.J. Pinfield, A.J. Burgasser, N. Lodieu, H.R.A. Jones, E.L. Martín, B. Burningham, D. Homeier, F. Allard, M.R. Zapatero Osorio, L.C. Smith, R.L. Smart, B. López Martí, F. Marocco and R. Rebolo |
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