File Download
  Links for fulltext
     (May Require Subscription)
Supplementary

Conference Paper: Chemical enrichment of the solar system by stellar ejecta

TitleChemical enrichment of the solar system by stellar ejecta
Authors
Kwok, S
Issue Date2015
PublisherCambridge University Press. The Journal's web site is located at http://journals.cambridge.org/action/displayJournal?jid=IAU
Citation
The 28th International Astronomical Union (IAU) General Assembly, Beijing, China, 20-31 August 2012. In International Astronomical Union Proceedings, 2015, v. 10, p. 161 How to Cite?
DOI: http://dx.doi.org/10.1017/S174392131400516X
AbstractSpectroscopic observations of evolved stars have shown signatures of aromatic and aliphatic compounds. This suggests that complex organics with chemical structures similar to those of insoluble organic matter (IOM) found in carbonaceous meteorites are made in stars. This raises the possibility that in addition to known pre-solar grains such as silicon carbide, organic star dust may also have traveled across the Galaxy to the Solar System.
DescriptionSpecial Sessions (GA) - SpS12 (27-30 August 2012) Theme: Modern views of the interstellar medium
Talks
Persistent Identifierhttp://hdl.handle.net/10722/220541
ISSN
1743-9213
2020 SCImago Journal Rankings: 0.124

 

DC FieldValueLanguage
dc.contributor.authorKwok, S-
dc.date.accessioned2015-10-16T06:44:53Z-
dc.date.available2015-10-16T06:44:53Z-
dc.date.issued2015-
dc.identifier.citationThe 28th International Astronomical Union (IAU) General Assembly, Beijing, China, 20-31 August 2012. In International Astronomical Union Proceedings, 2015, v. 10, p. 161-
dc.identifier.issn1743-9213-
dc.identifier.urihttp://hdl.handle.net/10722/220541-
dc.descriptionSpecial Sessions (GA) - SpS12 (27-30 August 2012) Theme: Modern views of the interstellar medium-
dc.descriptionTalks-
dc.description.abstractSpectroscopic observations of evolved stars have shown signatures of aromatic and aliphatic compounds. This suggests that complex organics with chemical structures similar to those of insoluble organic matter (IOM) found in carbonaceous meteorites are made in stars. This raises the possibility that in addition to known pre-solar grains such as silicon carbide, organic star dust may also have traveled across the Galaxy to the Solar System.-
dc.languageeng-
dc.publisherCambridge University Press. The Journal's web site is located at http://journals.cambridge.org/action/displayJournal?jid=IAU-
dc.relation.ispartofInternational Astronomical Union Proceedings-
dc.rightsInternational Astronomical Union Proceedings. Copyright © Cambridge University Press.-
dc.titleChemical enrichment of the solar system by stellar ejecta-
dc.typeConference_Paper-
dc.identifier.emailKwok, S: deannote@hku.hk-
dc.identifier.authorityKwok, S=rp00716-
dc.description.naturepostprint-
dc.identifier.doi10.1017/S174392131400516X-
dc.identifier.scopuseid_2-s2.0-84981167249-
dc.identifier.hkuros255687-
dc.identifier.volume10-
dc.identifier.spage161-
dc.identifier.epage161-
dc.publisher.placeUnited Kingdom-
dc.identifier.issnl1743-9213-

Export via OAI-PMH Interface in XML Formats

OR

Export to Other Non-XML Formats