Primeval very low-mass stars and brown dwarfs: IV. New L subdwarfs, Gaia astrometry, population properties, and a blue brown dwarf binary

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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

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Bibliographic Details
Main Authors:	Zhang, Zeng Hua (Author) , Homeier, Derek (Author)
Format:	Article (Journal)
Language:	English
Published:	2018 July 31
In:	Monthly notices of the Royal Astronomical Society Year: 2018, Volume: 480, Issue: 4, Pages: 5447-5474
ISSN:	1365-2966
DOI:	10.1093/mnras/sty2054
Online Access:	Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty2054 Verlag, Volltext: https://academic.oup.com/mnras/article/480/4/5447/5062823
Author Notes:	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

Description
Summary:	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
Item Description:	Gesehen am 07.08.2020
Physical Description:	Online Resource
ISSN:	1365-2966
DOI:	10.1093/mnras/sty2054