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1999•Unpublished venueRequires access

Preliminary results on the circumstellar envelopes of alpha Ori and R Leo from CO 4.6 mu m line emission

N. Ryde, B. Gustafsson, KH Hinkle, Kimmo Eriksson, D. Lambert, H. Olofsson

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Abstract

CO 4.6 mu m vibration-rotational lines are detected in fluorescent emission from the inner regions of the Betelgeuse (a Orionis) and R Leonis stellar winds. The spatially and spectrally resolved 1-0 R(1), R(2), and R(3) line profiles are found to be highl

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What this paper is about

CO 4.6 mu m vibration-rotational lines are detected in fluorescent emission from the inner regions of the Betelgeuse (a Orionis) and R Leonis stellar winds. The spatially and spectrally resolved 1-0 R(1), R(2), and R(3) line profiles are found to be highl

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Available abstract

CO 4.6 mu m vibration-rotational lines are detected in fluorescent emission from the inner regions of the Betelgeuse (a Orionis) and R Leonis stellar winds. The spatially and spectrally resolved 1-0 R(1), R(2), and R(3) line profiles are found to be highl

Key concepts: Physics, Astrophysics, Emission spectrum, H-alpha, Line (geometry), Supergiant, Astronomical spectroscopy, Spectral line

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Preliminary results on the circumstellar envelopes of alpha Ori and R Leo from CO 4.6 mu m line emission — Research Paper | ScholarLens