C Vibration Rotation Lines from Circumstellar Shells

Details C Vibration Rotation Lines from Circumstellar Shells C Vibration Rotation Lines from Circumstellar Shells

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mlrg.proc...81s&link_type=abstract

Mass Loss from Red Giants; Proceedings of the Conference, University of California, Los Angeles, CA, June 20, 21, 1984. Edited

Astronomy and Astrophysics

Astrophysics

Scientific paper

The authors have conducted an investigation of the inner part (≡2 - 3arcsec) of red giant star envelopes through observations of emission in the 4.6 μm vibration rotation lines of CO produced by resonance scattering. A novel experimental technique, employing an annular aperture to mask the central infrared continuum source, was used to obtain line profiles at a mean angular offset of 2.7±0.7arcsec from the center. The results for the carbon-rich Mira variable IRC+10216 are presented.

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