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        Primeval very low-mass stars and brown dwarfs. I. Six new L subdwarfs, classification and atmospheric properties

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        Author
        Zhang, Z. H.
        Pinfield, D. J.
        Galvez-Ortiz, M. C.
        Burningham, B.
        Lodieu, N.
        Marocco, F.
        Burgasser, A. J.
        Day-Jones, A. C.
        Allard, F.
        Jones, H. R. A.
        Homeier, D.
        Gomes, J.
        Smart, R. L.
        Attention
        2299/18239
        Abstract
        We have conducted a search for L subdwarf candidates within the photometric catalogues of the UKIRT Infrared Deep Sky Survey and Sloan Digital Sky Survey. Six of our candidates are confirmed as L subdwarfs spectroscopically at optical and/or near infrared wavelengths. We also present new optical spectra of three previously known L subdwarfs (WISEA J001450.17-083823.4, 2MASS J00412179+3547133, ULAS J124425.75+102439.3). We examined the spectral types and metallicity subclasses classification of known L subdwarfs. We summarised the spectroscopic properties of L subdwarfs with different spectral types and subclasses. We classify these new L subdwarfs by comparing their spectra to known L subdwarfs and L dwarf standards. We estimate temperatures and metallicities of 22 late type M and L subdwarfs by comparing their spectra to BT-Settl models. We find that L subdwarfs have temperatures between 1500 K and 2700 K, which are higher than similarly-typed L dwarfs by around 100-400 K depending on different subclasses and subtypes. We constrained the metallicity ranges of subclasses of M, L and T subdwarfs. We also discussed the spectral type and absolute magnitude relationships for L and T subdwarfs.
        Publication date
        2017-01-01
        Published in
        Monthly Notices of the Royal Astronomical Society
        Published version
        https://doi.org/10.1093/mnras/stw2438
        Other links
        http://hdl.handle.net/2299/18239
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