Published 1997
| public
Book Section - Chapter
Pre-Shock and post-shock abundance ratios of atomic carbon to CO in IC 443 G
Abstract
IC 443 is a prominent, well-studied supernova remnant. Optical pictures show multiple filaments through the midst of which runs a lane of extinction. Bright H₂ emission marks the region of interaction between the SNR and the foreground cloud. Clump G is at the western side of the SNR and is heavily obscured. At its position the velocity of supernova shock is nearly in the plane of the sky and the radial velocity of the shocked material is displaced very little from that of the ambient foreground material.
Additional Information
© Springer Science+Business Media Dordrecht 1997. The Caltech Submillimeter Observatory is supported by the National Science Foundation under grant AST 93-13929. We thank K. M. Merrill for permission to use the H2 image before publication.Additional details
- Eprint ID
- 106761
- DOI
- 10.1007/978-94-011-5414-7_68
- Resolver ID
- CaltechAUTHORS:20201120-120817212
- AST 93-13929
- NSF
- Created
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2020-11-23Created from EPrint's datestamp field
- Updated
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2021-11-16Created from EPrint's last_modified field
- Series Name
- IAU Symposium Proceedings Series
- Series Volume or Issue Number
- 170