Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/9649
Title: Methane band and Spitzer mid-IR imaging of L and T dwarf candidates in the Pleiades
Authors: Casewell, S. L.
Jameson, Richard F.
Burleigh, M. R.
Dobbie, P. D.
Roy, Mervyn
Hodgkin, S. T.
Moraux, E.
First Published: 11-Apr-2011
Publisher: Oxford University Press for the Royal Astronomical Society
Citation: Monthly Notices of the Royal Astronomical Society, 2011, 412 (3), pp. 2071-2078.
Abstract: We present Spitzer observations at [3.6] and [4.5] μm together with the methane short (1.58 μm) − methane long (1.69 μm) colour for three cool dwarfs in the Pleiades, PLZJ23, PLZJ93 and PLZJ100. We determine the effective temperatures of PLZJ23 and PLZJ93 to be ≈1200 and ≈1100 K. From the broad-band photometry we place an upper limit of 1100K on the effective temperature of PLZJ100 but lack the data required to determine the value more precisely. These temperatures are in the T dwarf regime, yet the methane colours indicate no methane is present.We attribute this to youth/low gravity in line with theoretical expectations. However, we find even less methane is present than predicted by the models. PLZJ23 and PLZJ93 are also very bright in the [3.6] μm waveband (PLZJ100 is not measured) compared to field brown dwarfs which can also be explained by this lack of methane. The definition of the T spectral class is the appearance of methane absorption, so strictly, via this definition, PLZJ93 and PLZJ100 cannot be described as T dwarfs. The colours of these two objects are, however, not compatible with those of L dwarfs. Thus we have a classification problem and cannot assign these objects a (photometric) spectral type.
DOI Link: 10.1111/j.1365-2966.2010.18044.x
ISSN: 0035-8711
eISSN: 1365-2966
Links: http://mnras.oxfordjournals.org/content/412/3/2071.abstract
http://hdl.handle.net/2381/9649
Version: Publisher Version
Status: Peer-reviewed
Type: Article
Rights: Copyright © 2011 The Authors, Monthly Notices of the Royal Astronomical Society © 2011 RAS. Deposited with reference to the publisher's archiving policy available on the publisher's website.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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