Acetone in Orion BN/KL - High-resolution maps of a special oxygen-bearing molecule
hal.structure.identifier | FORMATION STELLAIRE 2013 | |
dc.contributor.author | PENG, T.-C. | |
hal.structure.identifier | FORMATION STELLAIRE 2013 | |
dc.contributor.author | DESPOIS, D. | |
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'Astrophysique de Bordeaux [Pessac] [LAB] | |
hal.structure.identifier | Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB] | |
dc.contributor.author | BROUILLET, N. | |
hal.structure.identifier | FORMATION STELLAIRE 2013 | |
dc.contributor.author | BAUDRY, Alain | |
dc.contributor.author | FAVRE, C. | |
dc.contributor.author | REMIJAN, A. | |
dc.contributor.author | WOOTTEN, A. | |
dc.contributor.author | WILSON, T. L. | |
hal.structure.identifier | Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA] | |
dc.contributor.author | COMBES, F. | |
dc.contributor.author | WLODARCZAK, G. | |
dc.date.created | 2013-04-17 | |
dc.date.issued | 2013 | |
dc.identifier.issn | 0004-6361 | |
dc.description.abstractEn | As one of the prime targets of interstellar chemistry study, Orion BN/KL clearly shows different molecular distributions between large nitrogen- (e.g., C2H5CN) and oxygen-bearing (e.g., HCOOCH3) molecules. However, acetone (CH3)2CO, a special complex O-bearing molecule, has been shown to have a very different distribution from other typical O-bearing molecules in the BN/KL region. We searched for acetone within our IRAM Plateau de Bure Interferometer 3 mm and 1.3 mm data sets. Twenty-two acetone lines were searched within these data sets. The angular resolution ranged from 1.8 X 0.8 to 6.0 X 2.3 arcsec^2, and the spectral resolution ranged from 0.4 to 1.9 km s-1. Nine of the acetone lines appear free of contamination. Three main acetone peaks (Ace-1, 2, and 3) are identified in Orion BN/KL. The new acetone source Ace-3 and the extended emission in the north of the hot core region have been found for the first time. An excitation temperature of about 150 K is determined toward Ace-1 and Ace-2, and the acetone column density is estimated to be 2-4 X 10^16 cm-2 with a relative abundance of 1-6 X 10^-8 toward these two peaks. Acetone is a few times less abundant toward the hot core and Ace-3 compared with Ace-1 and Ace-2. We find that the overall distribution of acetone in BN/KL is similar to that of N-bearing molecules, e.g., NH3 and C2H5CN, and very different from those of large O-bearing molecules, e.g., HCOOCH3 and (CH3)2O. Our findings show the acetone distribution is more extended than in previous studies and does not originate only in those areas where both N-bearing and O-bearing species are present. Moreover, because the N-bearing molecules may be associated with shocked gas in Orion BN/KL, this suggests that the formation and/or destruction of acetone may involve ammonia or large N-bearing molecules in a shocked-gas environment. | |
dc.language.iso | en | |
dc.publisher | EDP Sciences | |
dc.title.en | Acetone in Orion BN/KL - High-resolution maps of a special oxygen-bearing molecule | |
dc.type | Article de revue | |
dc.identifier.doi | 10.1051/0004-6361/201220891 | |
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 | 1304.4793 | |
bordeaux.journal | Astronomy and Astrophysics - A&A | |
bordeaux.page | id.A78 | |
bordeaux.volume | 554 | |
bordeaux.peerReviewed | oui | |
hal.identifier | hal-00822073 | |
hal.version | 1 | |
hal.popular | non | |
hal.audience | Internationale | |
hal.origin.link | https://hal.archives-ouvertes.fr//hal-00822073v1 | |
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