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|Title: ||The spectrum of TMR-1C is consistent with a background star|
|Authors: ||Terebey, S.|
Van Buren, D.
Padgett, D. L.
|Keywords: ||circumstellar matter|
|Issue Date: ||May-2000 |
|Publisher: ||The American Astronomical Society|
|Citation: ||The Astronomical Journal, 119:2341-2348, 2000 May|
|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. ...|
|Appears in Collections:||JPL TRS 1992+|
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