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The spectrum of TMR-1C is consistent with a background star

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dc.contributor.author Terebey, S.
dc.contributor.author Van Buren, D.
dc.contributor.author Matthews, K.
dc.contributor.author Padgett, D. L.
dc.date.accessioned 2008-10-08T21:54:39Z
dc.date.available 2008-10-08T21:54:39Z
dc.date.issued 2000-05
dc.identifier.citation The Astronomical Journal, 119:2341-2348, 2000 May en_US
dc.identifier.clearanceno 00-0537
dc.identifier.uri http://hdl.handle.net/2014/40978
dc.description.abstract ...This paper presents near-infrared grism spectroscopy to constrain the efective temperature of TMR-1C, obtained with the Near-Infrared Camera (NIRC) at Keck Observatory. To interpret the data, we construct a grid of extincted M dwarf spectra to compare with the low-resolution (RD120) NIRC spectrum. The assumed extinction corresponds to standard interstellar dust. With the additional assumption that no near-infrared dust excess contributes to the spectrum, then M4.5 is the latest spectral type TMR-1C can have within the uncertainties. ... en_US
dc.description.sponsorship NASA/JPL en_US
dc.language.iso en_US en_US
dc.publisher The American Astronomical Society en_US
dc.subject circumstellar matter en_US
dc.subject infrared radiation en_US
dc.subject planetary systems en_US
dc.title The spectrum of TMR-1C is consistent with a background star en_US
dc.type Article en_US


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