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The Astrophysical Journal
Article . 1997 . Peer-reviewed
Data sources: Crossref
https://dx.doi.org/10.48550/ar...
Article . 1997
License: arXiv Non-Exclusive Distribution
Data sources: Datacite
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Neutral Carbon in the Protoplanetary Nebulae CRL 618 and CRL 2688

Authors: Young, K.;

Neutral Carbon in the Protoplanetary Nebulae CRL 618 and CRL 2688

Abstract

The 609u 3P1 -> 3P0 line of neutral atomic carbon has been detected in the protoplanetary nebulae CRL 618 and CRL 2688. CI appears to be about 7% as abundant as CO in CRL 2688, and 70% as abundant as CO in CRL 618. CI emission arises primarily from the slow component of the wind from these objects. The data presented here indicate that CI gradually becomes more abundant as the star leaves the AGB, and CI is significantly enhanced relative to CO before the star develops a large HII region.

7 pages, LaTex AASTeX macros. To appear in ApJ Letters

Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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    popularity
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    influence
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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
18
Average
Average
Average
Green
bronze