NAYLOR, D. A.; DARTOIS, E.; HABART, E.; ABERGEL, A.; BALUTEAU, J.-P.; JONES, S. C.; POLEHAMPTON, E.; ADE, P.; ANDERSON, L. D.; ANDRÉ, P.; ARAB, H.; BERNARD, J.-P.; BLAGRAVE, K.; BONTEMPS, Sylvain; BOULANGER, F.; COHEN, M.; COMPIÈGNE, M.; COX, P.; DAVIS, G.; EMERY, R.; FULTON, T.; GRY, C.; HUANG, M.; JOBLIN, C.; KIRK, J. M.; LAGACHE, Guilaine; LIM, T.; MADDEN, S.; MAKIWA, G.; MARTIN, P.; MIVILLE-DESCHÊNES, M.-A.; MOLINARI, S.; MOSELEY, H.; MOTTE, F.; OKUMURA, K.; PINHEIRO GONÇALVES, D.; RODÓN, J. A.; RUSSEIL, D.; SARACENO, P.; SIDHER, S.; SPENCER, L.; SWINYARD, B.; WARD-THOMPSON, D.; WHITE, G. J.; ZAVAGNO, Annie

doi:10.1051/0004-6361/201014656

dc.contributor.author	NAYLOR, D. A.
hal.structure.identifier	Institut d'astrophysique spatiale [IAS]
dc.contributor.author	DARTOIS, E.
hal.structure.identifier	Institut d'astrophysique spatiale [IAS]
dc.contributor.author	HABART, E.
hal.structure.identifier	Institut d'astrophysique spatiale [IAS]
dc.contributor.author	ABERGEL, A.
dc.contributor.author	BALUTEAU, J.-P.
dc.contributor.author	JONES, S. C.
dc.contributor.author	POLEHAMPTON, E.
dc.contributor.author	ADE, P.
hal.structure.identifier	Laboratoire d'Astrophysique de Marseille [LAM]
dc.contributor.author	ANDERSON, L. D.
hal.structure.identifier	Laboratoire d'Informatique de Nantes Atlantique [LINA]
dc.contributor.author	ANDRÉ, P.
dc.contributor.author	ARAB, H.
hal.structure.identifier	Institut d'astrophysique spatiale [IAS]
hal.structure.identifier	Centre d'étude spatiale des rayonnements [CESR]
dc.contributor.author	BERNARD, J.-P.
dc.contributor.author	BLAGRAVE, K.
hal.structure.identifier	Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
hal.structure.identifier	Observatoire aquitain des sciences de l'univers [OASU]
hal.structure.identifier	Université Sciences et Technologies - Bordeaux 1 [UB]
hal.structure.identifier	Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
dc.contributor.author	BONTEMPS, Sylvain
hal.structure.identifier	Institut d'astrophysique spatiale [IAS]
dc.contributor.author	BOULANGER, F.
dc.contributor.author	COHEN, M.
dc.contributor.author	COMPIÈGNE, M.
dc.contributor.author	COX, P.
hal.structure.identifier	Department of Ecology and Evolutionary Biology [Princeton]
dc.contributor.author	DAVIS, G.
dc.contributor.author	EMERY, R.
dc.contributor.author	FULTON, T.
hal.structure.identifier	Laboratoire d'Astrophysique de Marseille [LAM]
dc.contributor.author	GRY, C.
hal.structure.identifier	National Astronomical Observatories [Beijing] [NAOC]
dc.contributor.author	HUANG, M.
hal.structure.identifier	Centre d'étude spatiale des rayonnements [CESR]
dc.contributor.author	JOBLIN, C.
dc.contributor.author	KIRK, J. M.
hal.structure.identifier	Institut d'astrophysique spatiale [IAS]
dc.contributor.author	LAGACHE, Guilaine
hal.structure.identifier	Laboratoire de Probabilités et Modèles Aléatoires [LPMA]
dc.contributor.author	LIM, T.
hal.structure.identifier	Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée [DAPNIA]
dc.contributor.author	MADDEN, S.
dc.contributor.author	MAKIWA, G.
hal.structure.identifier	CITA
dc.contributor.author	MARTIN, P.
hal.structure.identifier	Institut d'astrophysique spatiale [IAS]
dc.contributor.author	MIVILLE-DESCHÊNES, M.-A.
hal.structure.identifier	Istituto di Fisica dello Spazio Interplanetario [IFSI]
dc.contributor.author	MOLINARI, S.
dc.contributor.author	MOSELEY, H.
hal.structure.identifier	Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
hal.structure.identifier	Institut de Recherches sur les lois Fondamentales de l'Univers [IRFU]
dc.contributor.author	MOTTE, F.
dc.contributor.author	OKUMURA, K.
dc.contributor.author	PINHEIRO GONÇALVES, D.
dc.contributor.author	RODÓN, J. A.
hal.structure.identifier	Laboratoire d'Astrophysique de Marseille [LAM]
dc.contributor.author	RUSSEIL, D.
hal.structure.identifier	Istituto di Fisica dello Spazio Interplanetario [IFSI]
dc.contributor.author	SARACENO, P.
dc.contributor.author	SIDHER, S.
dc.contributor.author	SPENCER, L.
dc.contributor.author	SWINYARD, B.
hal.structure.identifier	School of Physics and Astronomy [Cardiff]
dc.contributor.author	WARD-THOMPSON, D.
hal.structure.identifier	Engineering Department
dc.contributor.author	WHITE, G. J.
hal.structure.identifier	Laboratoire d'Astrophysique de Marseille [LAM]
hal.structure.identifier	Observatoire Astronomique de Marseille Provence [OAMP]
dc.contributor.author	ZAVAGNO, Annie
dc.date.created	2010
dc.date.issued	2010
dc.identifier.issn	0004-6361
dc.description.abstractEn	Aims: To follow the species chemistry arising in diverse sources of the Galaxy with Herschel. Methods: SPIRE FTS sparse sampled maps of the Orion bar & compact HII regions G29.96-0.02 and G32.80+0.19 have been analyzed. Results: Beyond the wealth of atomic and molecular lines detected in the high-resolution spectra obtained with the FTS of SPIRE in the Orion Bar, one emission line is found to lie at the position of the fundamental rotational transition of CH+ as measured precisely in the laboratory by Pearson and Drouion. This coincidence suggests that it is the first detection of the fundamental rotational transition of CH+. This claim is strengthened by the observation of the lambda doublet transitions arising from its relative, CH, which are also observed in the same spectrum. The broad spectral coverage of the SPIRE FTS allows for the simultaneous measurement of these closely related chemically species, under the same observing conditions. The importance of these lines are discussed and a comparison with results obtained from models of the photon dominated region (PDR) of Orion are presented. The CH+ line also appears in absorption in the spectra of the two galactic compact HII regions G29.96-0.02 and G32.80+0.19, which is likely due to the presence of CH+ in the the cold neutral medium of the galactic plane. These detections will shed light on the formation processes and on the existence of CH+, which are still outstanding questions in astrophysics. Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.
dc.language.iso	en
dc.publisher	EDP Sciences
dc.subject.en	ISM: molecules
dc.subject.en	evolution
dc.subject.en	ISM: general
dc.subject.en	space vehicles: instruments
dc.subject.en	techniques: spectroscopic
dc.title.en	First detection of the methylidyne cation (CH+) fundamental rotational line with the Herschel/SPIRE FTS
dc.type	Article de revue
dc.identifier.doi	10.1051/0004-6361/201014656
dc.subject.hal	Planète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
dc.subject.hal	Physique [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
dc.identifier.arxiv	1005.1916
bordeaux.journal	Astronomy and Astrophysics - A&A
bordeaux.page	L117
bordeaux.volume	518
bordeaux.peerReviewed	oui
hal.identifier	hal-00522987
hal.version	1
hal.popular	non
hal.audience	Internationale
hal.origin.link	https://hal.archives-ouvertes.fr//hal-00522987v1
bordeaux.COinS	ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Astronomy%20and%20Astrophysics%20-%20A&A&rft.date=2010&rft.volume=518&rft.spage=L117&rft.epage=L117&rft.eissn=0004-6361&rft.issn=0004-6361&rft.au=NAYLOR,%20D.%20A.&DARTOIS,%20E.&HABART,%20E.&ABERGEL,%20A.&BALUTEAU,%20J.-P.&rft.genre=article

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First detection of the methylidyne cation (CH+) fundamental rotational line with the Herschel/SPIRE FTS

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