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1999•Unpublished venueRequires access

Resolved CO 4.6 um Line Emission from Inner Circumstellar Envelopes -- the Case of Mira

N. Ryde, Kimmo Eriksson, B. Gustafsson, Kenneth H. Hinkle, D. L. Lambert, H. Olofsson, F. L. Schöier

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Abstract

The 13-16 mu m region observed by the Infrared Space Observatory (ISO) of several ABG stars are discussed. We present and analyse spectra of seven M giants which show carbon dioxide features. To explain the features of the bands, we suggest they originate

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What this paper is about

The 13-16 mu m region observed by the Infrared Space Observatory (ISO) of several ABG stars are discussed. We present and analyse spectra of seven M giants which show carbon dioxide features. To explain the features of the bands, we suggest they originate

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Available abstract

The 13-16 mu m region observed by the Infrared Space Observatory (ISO) of several ABG stars are discussed. We present and analyse spectra of seven M giants which show carbon dioxide features. To explain the features of the bands, we suggest they originate

Key concepts: Astrophysics, Physics, Observatory, Stars, Circumstellar envelope, Astronomy, Emission spectrum, Carbon star

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