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Pre-Shock and post-shock abundance ratios of atomic carbon to CO in IC 443 G

Keene, Jocelyn and Phillips, T. G. and Van Dishoeck, Ewine F. (1997) Pre-Shock and post-shock abundance ratios of atomic carbon to CO in IC 443 G. In: CO: Twenty-Five Years of Millimeter-Wave Spectroscopy. IAU Symposium Proceedings Series. No.170. Springer Netherlands , Dordrecht, pp. 382-384. ISBN 9780792342847. https://resolver.caltech.edu/CaltechAUTHORS:20201120-120817212

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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.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1007/978-94-011-5414-7_68DOIArticle
https://rdcu.be/ca730PublisherFree ReadCube access
ORCID:
AuthorORCID
Van Dishoeck, Ewine F.0000-0001-7591-1907
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.
Funders:
Funding AgencyGrant Number
NSFAST 93-13929
Series Name:IAU Symposium Proceedings Series
Issue or Number:170
Record Number:CaltechAUTHORS:20201120-120817212
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20201120-120817212
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:106761
Collection:CaltechAUTHORS
Deposited By: Rebecca Minjarez
Deposited On:23 Nov 2020 16:43
Last Modified:23 Nov 2020 16:43

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