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Conference Paper: The chemical composition of 9P/tempel 1 from radio observations

TitleThe chemical composition of 9P/tempel 1 from radio observations
Authors
Crovisier, JBiver, NBockeléeMorvan, DBoissier, JColom, PLecacheux, AMoreno, RPaubert, GLis, DCSumner, MFrisk, UHjalmarson, ÅOlberg, MWinnberg, AFlorén, HSandqvist, AKwok, S
Issue Date2009
Citation
Eso Astrophysics Symposia, 2009, v. 2009, p. 243-248 How to Cite?
DOI: http://dx.doi.org/10.1007/978-3-540-76959-0_32
AbstractIn 2005, as part of a world-wide multi-wavelength investigation of comet 9P/Tempel 1 in support to the Deep Impact mission, we conducted radio spectroscopic observations with the Nançay radio telescope, the Odin satellite, the CSO 10-m and the IRAM 30-m telescopes. We report here our results concerning the chemical composition of the comet. The relative abundances of the detected species (H 2O, CH 3OH, H 2S, HCN) or their upper limits (CO, H 2CO, CS) are comparable to the mean values observed in other comets. No significant changes of the outgassing rates (except possibly for CH 3OH) or of the molecular abundances were observed following the impact. © 2009 Springer-Verlag Berlin Heidelberg.
Persistent Identifierhttp://hdl.handle.net/10722/179624
ISSN
1431-2433
ISI Accession Number ID
WOS:000262404900032
References
References in Scopus

 

DC FieldValueLanguage
dc.contributor.authorCrovisier, Jen_US
dc.contributor.authorBiver, Nen_US
dc.contributor.authorBockeléeMorvan, Den_US
dc.contributor.authorBoissier, Jen_US
dc.contributor.authorColom, Pen_US
dc.contributor.authorLecacheux, Aen_US
dc.contributor.authorMoreno, Ren_US
dc.contributor.authorPaubert, Gen_US
dc.contributor.authorLis, DCen_US
dc.contributor.authorSumner, Men_US
dc.contributor.authorFrisk, Uen_US
dc.contributor.authorHjalmarson, Åen_US
dc.contributor.authorOlberg, Men_US
dc.contributor.authorWinnberg, Aen_US
dc.contributor.authorFlorén, Hen_US
dc.contributor.authorSandqvist, Aen_US
dc.contributor.authorKwok, Sen_US
dc.date.accessioned2012-12-19T10:01:41Z-
dc.date.available2012-12-19T10:01:41Z-
dc.date.issued2009en_US
dc.identifier.citationEso Astrophysics Symposia, 2009, v. 2009, p. 243-248en_US
dc.identifier.issn1431-2433en_US
dc.identifier.urihttp://hdl.handle.net/10722/179624-
dc.description.abstractIn 2005, as part of a world-wide multi-wavelength investigation of comet 9P/Tempel 1 in support to the Deep Impact mission, we conducted radio spectroscopic observations with the Nançay radio telescope, the Odin satellite, the CSO 10-m and the IRAM 30-m telescopes. We report here our results concerning the chemical composition of the comet. The relative abundances of the detected species (H 2O, CH 3OH, H 2S, HCN) or their upper limits (CO, H 2CO, CS) are comparable to the mean values observed in other comets. No significant changes of the outgassing rates (except possibly for CH 3OH) or of the molecular abundances were observed following the impact. © 2009 Springer-Verlag Berlin Heidelberg.en_US
dc.languageengen_US
dc.relation.ispartofESO Astrophysics Symposiaen_US
dc.titleThe chemical composition of 9P/tempel 1 from radio observationsen_US
dc.typeConference_Paperen_US
dc.identifier.emailKwok, S: deannote@hku.hken_US
dc.identifier.authorityKwok, S=rp00716en_US
dc.description.naturelink_to_subscribed_fulltexten_US
dc.identifier.doi10.1007/978-3-540-76959-0_32en_US
dc.identifier.scopuseid_2-s2.0-54849416356en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-54849416356&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume2009en_US
dc.identifier.spage243en_US
dc.identifier.epage248en_US
dc.identifier.isiWOS:000262404900032-
dc.publisher.placeGermanyen_US
dc.identifier.scopusauthoridCrovisier, J=35448565400en_US
dc.identifier.scopusauthoridBiver, N=6603734959en_US
dc.identifier.scopusauthoridBockeléeMorvan, D=7003530700en_US
dc.identifier.scopusauthoridBoissier, J=7101971162en_US
dc.identifier.scopusauthoridColom, P=6603805418en_US
dc.identifier.scopusauthoridLecacheux, A=7003423533en_US
dc.identifier.scopusauthoridMoreno, R=7202177731en_US
dc.identifier.scopusauthoridPaubert, G=6701489710en_US
dc.identifier.scopusauthoridLis, DC=7005226300en_US
dc.identifier.scopusauthoridSumner, M=10638914800en_US
dc.identifier.scopusauthoridFrisk, U=8966521600en_US
dc.identifier.scopusauthoridHjalmarson, Å=15744175200en_US
dc.identifier.scopusauthoridOlberg, M=16201342800en_US
dc.identifier.scopusauthoridWinnberg, A=6603734778en_US
dc.identifier.scopusauthoridFlorén, H=6602447564en_US
dc.identifier.scopusauthoridSandqvist, A=35451841800en_US
dc.identifier.scopusauthoridKwok, S=22980498300en_US
dc.identifier.issnl1431-2433-

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