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Please use this identifier to cite or link to this item:
http://hdl.handle.net/2014/40978
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| Title: | The spectrum of TMR-1C is consistent with a background star |
| Authors: | Terebey, S.
Van Buren, D.
Matthews, K.
Padgett, D. L. |
| Keywords: | circumstellar matter
infrared radiation
planetary systems |
| 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. ... |
| URI: | http://hdl.handle.net/2014/40978 |
| Appears in Collections: | JPL TRS 1992+
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