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Article: On the viability of the pah model as an explanation of the unidentified infrared emission features

TitleOn the viability of the pah model as an explanation of the unidentified infrared emission features
Authors
Zhang, YKwok, S
KeywordsInfrared: Ism
Ism: General
Ism: Lines and bands
Ism: Molecules
Issue Date2014
Citation
The Astrophysical Journal, 2014, v. 798 n. 1, article no. 37 How to Cite?
DOI: http://dx.doi.org/10.1088/0004-637X/798/1/37
Persistent Identifierhttp://hdl.handle.net/10722/207730
ISI Accession Number ID
WOS:000347245100034

 

DC FieldValueLanguage
dc.contributor.authorZhang, Yen_US
dc.contributor.authorKwok, Sen_US
dc.date.accessioned2015-01-19T09:38:56Z-
dc.date.available2015-01-19T09:38:56Z-
dc.date.issued2014en_US
dc.identifier.citationThe Astrophysical Journal, 2014, v. 798 n. 1, article no. 37en_US
dc.identifier.urihttp://hdl.handle.net/10722/207730-
dc.languageengen_US
dc.relation.ispartofThe Astrophysical Journalen_US
dc.subjectInfrared: Ism-
dc.subjectIsm: General-
dc.subjectIsm: Lines and bands-
dc.subjectIsm: Molecules-
dc.titleOn the viability of the pah model as an explanation of the unidentified infrared emission featuresen_US
dc.typeArticleen_US
dc.identifier.emailZhang, Y: zhangy96@hku.hken_US
dc.identifier.emailKwok, S: deannote@hku.hken_US
dc.identifier.authorityZhang, Y=rp00841en_US
dc.identifier.authorityKwok, S=rp00716en_US
dc.description.naturepublished_or_final_version-
dc.identifier.doi10.1088/0004-637X/798/1/37en_US
dc.identifier.scopuseid_2-s2.0-84919470965-
dc.identifier.hkuros242098en_US
dc.identifier.volume798en_US
dc.identifier.spagearticle no. 37en_US
dc.identifier.epagearticle no. 37en_US
dc.identifier.eissn1538-4357-
dc.identifier.isiWOS:000347245100034-
dc.identifier.issnl0004-637X-

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