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Article: The far-infrared colors of carbon stars revisited
Title | The far-infrared colors of carbon stars revisited |
---|---|
Authors | |
Keywords | Infrared: Stars Stars: Carbon Stars: Circumstellar Matter Stars: Evolution Stars: Mass Loss |
Issue Date | 1996 |
Publisher | E D P Sciences. The Journal's web site is located at http://www.aanda.org |
Citation | Astronomy And Astrophysics, 1996, v. 308 n. 3, p. 738-746 How to Cite? |
Abstract | In view of recent developments in the theory of carbon star evolution it has become necessary to re-examine the source of the excess 100 μm flux associated with carbon stars. We demonstrate that the observed far infrared colors of carbon stars are not due to cirrus contamination and that a geometrically thin detached shell provides insufficient far-IR flux to match the observations. We also show that more recent models are consistent with a geometrically thick detached shell. |
Persistent Identifier | http://hdl.handle.net/10722/179644 |
ISSN | 2023 Impact Factor: 5.4 2023 SCImago Journal Rankings: 1.896 |
References |
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Egan, MP | en_US |
dc.contributor.author | Kwok, S | en_US |
dc.contributor.author | Leung, CM | en_US |
dc.contributor.author | Price, SD | en_US |
dc.date.accessioned | 2012-12-19T10:02:14Z | - |
dc.date.available | 2012-12-19T10:02:14Z | - |
dc.date.issued | 1996 | en_US |
dc.identifier.citation | Astronomy And Astrophysics, 1996, v. 308 n. 3, p. 738-746 | en_US |
dc.identifier.issn | 0004-6361 | en_US |
dc.identifier.uri | http://hdl.handle.net/10722/179644 | - |
dc.description.abstract | In view of recent developments in the theory of carbon star evolution it has become necessary to re-examine the source of the excess 100 μm flux associated with carbon stars. We demonstrate that the observed far infrared colors of carbon stars are not due to cirrus contamination and that a geometrically thin detached shell provides insufficient far-IR flux to match the observations. We also show that more recent models are consistent with a geometrically thick detached shell. | en_US |
dc.language | eng | en_US |
dc.publisher | E D P Sciences. The Journal's web site is located at http://www.aanda.org | en_US |
dc.relation.ispartof | Astronomy and Astrophysics | en_US |
dc.subject | Infrared: Stars | en_US |
dc.subject | Stars: Carbon | en_US |
dc.subject | Stars: Circumstellar Matter | en_US |
dc.subject | Stars: Evolution | en_US |
dc.subject | Stars: Mass Loss | en_US |
dc.title | The far-infrared colors of carbon stars revisited | en_US |
dc.type | Article | en_US |
dc.identifier.email | Kwok, S: deannote@hku.hk | en_US |
dc.identifier.authority | Kwok, S=rp00716 | en_US |
dc.description.nature | link_to_subscribed_fulltext | en_US |
dc.identifier.scopus | eid_2-s2.0-0010202303 | en_US |
dc.relation.references | http://www.scopus.com/mlt/select.url?eid=2-s2.0-0010202303&selection=ref&src=s&origin=recordpage | en_US |
dc.identifier.volume | 308 | en_US |
dc.identifier.issue | 3 | en_US |
dc.identifier.spage | 738 | en_US |
dc.identifier.epage | 746 | en_US |
dc.publisher.place | France | en_US |
dc.identifier.scopusauthorid | Egan, MP=7102009982 | en_US |
dc.identifier.scopusauthorid | Kwok, S=22980498300 | en_US |
dc.identifier.scopusauthorid | Leung, CM=7402612699 | en_US |
dc.identifier.scopusauthorid | Price, SD=7202475351 | en_US |
dc.identifier.issnl | 0004-6361 | - |