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Article: The far-infrared colors of carbon stars revisited

TitleThe far-infrared colors of carbon stars revisited
Authors
KeywordsInfrared: Stars
Stars: Carbon
Stars: Circumstellar Matter
Stars: Evolution
Stars: Mass Loss
Issue Date1996
PublisherE 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?
AbstractIn 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 Identifierhttp://hdl.handle.net/10722/179644
ISSN
2014 Impact Factor: 4.378
2015 SCImago Journal Rankings: 2.446
References

 

DC FieldValueLanguage
dc.contributor.authorEgan, MPen_US
dc.contributor.authorKwok, Sen_US
dc.contributor.authorLeung, CMen_US
dc.contributor.authorPrice, SDen_US
dc.date.accessioned2012-12-19T10:02:14Z-
dc.date.available2012-12-19T10:02:14Z-
dc.date.issued1996en_US
dc.identifier.citationAstronomy And Astrophysics, 1996, v. 308 n. 3, p. 738-746en_US
dc.identifier.issn0004-6361en_US
dc.identifier.urihttp://hdl.handle.net/10722/179644-
dc.description.abstractIn 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.languageengen_US
dc.publisherE D P Sciences. The Journal's web site is located at http://www.aanda.orgen_US
dc.relation.ispartofAstronomy and Astrophysicsen_US
dc.subjectInfrared: Starsen_US
dc.subjectStars: Carbonen_US
dc.subjectStars: Circumstellar Matteren_US
dc.subjectStars: Evolutionen_US
dc.subjectStars: Mass Lossen_US
dc.titleThe far-infrared colors of carbon stars revisiteden_US
dc.typeArticleen_US
dc.identifier.emailKwok, S: deannote@hku.hken_US
dc.identifier.authorityKwok, S=rp00716en_US
dc.description.naturelink_to_subscribed_fulltexten_US
dc.identifier.scopuseid_2-s2.0-0010202303en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-0010202303&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume308en_US
dc.identifier.issue3en_US
dc.identifier.spage738en_US
dc.identifier.epage746en_US
dc.publisher.placeFranceen_US
dc.identifier.scopusauthoridEgan, MP=7102009982en_US
dc.identifier.scopusauthoridKwok, S=22980498300en_US
dc.identifier.scopusauthoridLeung, CM=7402612699en_US
dc.identifier.scopusauthoridPrice, SD=7202475351en_US

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