Spectroscopic Study of Carbon Stars with the ISO-SWS |
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| Authors: | K Justtanont J Cami I Yamamura T De Jong LBFM Waters |
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| Institution: | (1) SRON, P.O.Box 800, 9700 AV Groningen, The Netherlands;(2) Department of Astronomy, University of Tokyo, 2-11-16 Yayoi, Bunkyo-ku, Tokyo 113, Japan;(3) Astronomical Institute, University of Amsterdam, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands |
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| Abstract: | We have observed ten carbon stars with different mass-loss rates using the Short Wavelength Spectrometer (SWS) on board ISO.
We found that not only the spectral energy distribution and the dust features, but that also that the strength and/or shape
of molecular absorption features in the infrared spectrum varies with the near-infrared color temperature, i.e. with the thickness
of the circumstellar envelope.
This revised version was published online in August 2006 with corrections to the Cover Date. |
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