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Article: Detection of C 60 in the protoplanetary nebula IRAS 01005+7910

TitleDetection of C 60 in the protoplanetary nebula IRAS 01005+7910
Authors
Zhang, YKwok, S
Keywordsinfrared: stars
stars: AGB and post-AGB
stars: circumstellar matter
Issue Date2011
PublisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205
Citation
Astrophysical Journal Letters, 2011, v. 730 n. 2 How to Cite?
DOI: http://dx.doi.org/10.1088/0004-637X/730/2/126
AbstractWe report the first detection of buckminsterfullerene (C 60) in a protoplanetary nebula. The vibrational transitions of C 60 at 7.0, 17.4, and 18.9μm are detected in the Spitzer/Infrared Spectrograph spectrum of IRAS 01005+7910. This detection suggests that fullerenes are formed shortly after the asymptotic giant branch but before the planetary nebulae stage. A comparison with the observations of C 60 in other sources is made and the implication for circumstellar chemistry is discussed. © 2011. The American Astronomical Society. All rights reserved.
Persistent Identifierhttp://hdl.handle.net/10722/135358
ISSN
2041-8205
2023 Impact Factor: 8.8
2023 SCImago Journal Rankings: 2.766
ISI Accession Number ID
WOS:000288441900066
Funding AgencyGrant Number
Research Grants Council of the Hong Kong Special Administrative Region, ChinaHKU7020/08P
Hong Kong University200909159007
Funding Information:

We are grateful to Peter Bernath for helpful discussions. We also thank Kris Sellgren, Jan Cami, and Jeronimo Bernard-Salas for providing the IRS spectra of NGC 7023 and Tc 1 from the their papers (Sellgren et al. 2010 and Cami et al. 2010). This work is based on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under a contract with NASA. This work was supported by a grant to S. K. from the Research Grants Council of the Hong Kong Special Administrative Region, China (project number HKU7020/08P) and a grant to Y.Z. from the Seed Funding Program for Basic Research in Hong Kong University (200909159007).

References
References in Scopus
Grants
The Infrared Morphologies of Planetary Nebulae

 

DC FieldValueLanguage
dc.contributor.authorZhang, Yen_HK
dc.contributor.authorKwok, Sen_HK
dc.date.accessioned2011-07-27T01:34:08Z-
dc.date.available2011-07-27T01:34:08Z-
dc.date.issued2011en_HK
dc.identifier.citationAstrophysical Journal Letters, 2011, v. 730 n. 2en_HK
dc.identifier.issn2041-8205en_HK
dc.identifier.urihttp://hdl.handle.net/10722/135358-
dc.description.abstractWe report the first detection of buckminsterfullerene (C 60) in a protoplanetary nebula. The vibrational transitions of C 60 at 7.0, 17.4, and 18.9μm are detected in the Spitzer/Infrared Spectrograph spectrum of IRAS 01005+7910. This detection suggests that fullerenes are formed shortly after the asymptotic giant branch but before the planetary nebulae stage. A comparison with the observations of C 60 in other sources is made and the implication for circumstellar chemistry is discussed. © 2011. The American Astronomical Society. All rights reserved.en_HK
dc.languageengen_US
dc.publisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205en_HK
dc.relation.ispartofAstrophysical Journal Lettersen_HK
dc.rightsThe Astrophysical Journal. Copyright © Institute of Physics Publishing, Inc.-
dc.subjectinfrared: starsen_HK
dc.subjectstars: AGB and post-AGBen_HK
dc.subjectstars: circumstellar matteren_HK
dc.titleDetection of C 60 in the protoplanetary nebula IRAS 01005+7910en_HK
dc.typeArticleen_HK
dc.identifier.openurlhttp://library.hku.hk:4550/resserv?sid=HKU:IR&issn=0004-637X&volume=730&issue=2, article no. 126&spage=&epage=&date=2011&atitle=Detection+of+C60+in+the+protoplanetary+nebula+IRAS+01005+7910-
dc.identifier.emailZhang, Y: zhangy96@hku.hken_HK
dc.identifier.emailKwok, S: deannote@hku.hken_HK
dc.identifier.authorityZhang, Y=rp00841en_HK
dc.identifier.authorityKwok, S=rp00716en_HK
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1088/0004-637X/730/2/126en_HK
dc.identifier.scopuseid_2-s2.0-79953698762en_HK
dc.identifier.hkuros186112en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-79953698762&selection=ref&src=s&origin=recordpageen_HK
dc.identifier.volume730en_HK
dc.identifier.issue2en_HK
dc.identifier.eissn1538-4357-
dc.identifier.isiWOS:000288441900066-
dc.publisher.placeUnited Kingdomen_HK
dc.relation.projectThe Infrared Morphologies of Planetary Nebulae-
dc.identifier.scopusauthoridZhang, Y=23768446500en_HK
dc.identifier.scopusauthoridKwok, S=22980498300en_HK

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