FAVRE, C.; WOOTTEN, H. A.; REMIJAN, A. J.; BROUILLET, N.; WILSON, T. L.; DESPOIS, D.; BAUDRY, Alain

doi:10.1088/2041-8205/739/1/L12

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FAVRE, C.
Observatoire aquitain des sciences de l'univers [OASU]
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
Université Sciences et Technologies - Bordeaux 1 [UB]
Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]

WOOTTEN, H. A.

REMIJAN, A. J.

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The Astrophysical journal letters. 2011, vol. 739, p. L12

Bristol : IOP Publishing

Résumé en anglais

We report the first subarcsecond (0farcs65 × 0farcs51) image of the dimethyl ether molecule, (CH3)2O, toward the Orion Kleinmann-Low nebula. The observations were carried at 43.4 GHz with the Expanded Very Large Array (EVLA). The distribution of the lower energy transition 61, 5-60, 6, EE (E u = 21 K) mapped in this study is in excellent agreement with the published dimethyl ether emission maps imaged with a lower resolution. The main emission peaks are observed toward the Compact Ridge and Hot Core southwest components, at the northern parts of the Compact Ridge and in an intermediate position between the Compact Ridge and the Hot Core. A notable result is that the distribution of dimethyl ether is very similar to that of another important larger O-bearing species, the methyl formate (HCOOCH3), imaged at a lower resolution. Our study shows that higher spectral resolution (WIDAR correlator) and increased spectral coverage provided by the EVLA offer new possibilities for imaging complex molecular species. The sensitivity improvement and the other EVLA improvements make this instrument well suited for high sensitivity, high angular resolution, and molecular line imaging.< Réduire

Mots clés en anglais

ISM: individual objects: Orion-KL

ISM: jets and outflows

ISM: molecules

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High-resolution Expanded Very Large Array Image of Dimethyl Ether (CH3)2O in Orion-KL

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