BRON, E.; DAUDON, C.; PETY, J.; LEVRIER, F.; GERIN, M.; GRATIER, P.; ORKISZ, Jan; GUZMÁN, V.; BARDEAU, S.; GOICOECHEA, J. R.; LISZT, H.; OEBERG, K.; PERETTO, N.; SIEVERS, A.; TREMBLIN, Pascal

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BRON, E.
Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA]

DAUDON, C.

PETY, J.
Institut de RadioAstronomie Millimétrique [IRAM]

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2017

Résumé en anglais

Integrated line intensities maps (in the 9-12km/s range) of the Orion B molecular cloud in $^{12}$CO(1-0), $^{13}$CO(1-0), C$^{18}$O(1-0), CN(1-0), HCO$^+$(1-0), used as basis for the clustering analysis presented in the paper. Maps of the cluster attributions of each pixel resulting from the two clustering analyses presented (based on CO isotopes only, and based on CO isotopes, HCO$^+$ and CN) are also included. Description of the fits files: - ClustCO.fit : Cluster assignation map from the clustering analysis based on CO isotopes only. - ClustFUV.fit : Cluster assignation map from the clustering analysis based on CO isotopes, HCO+ and CN. - map$^{12}$CO.fit : Integrated intensity (9-12km/s) map of the $^{12}$CO J=1-0 line. - map$^{13}$CO.fit : Integrated intensity (9-12km/s) map of the $^{13}$CO J=1-0 line. - mapC$^{18}$O.fit : Integrated intensity (9-12km/s) map of the C$^{18}$O J=1-0 line. - mapCN.fit : Integrated intensity (9-12km/s) map of the CN N=1-0 line. - mapHCOp.fit : Integrated intensity (9-12km/s) map of the HCO$^+$ J=1-0 line. (2 data files).< Réduire

Mots clés en anglais

Molecular clouds

Interstellar medium

Spectrophotometry

Carbon monoxide

Origine

Importé de hal

Unités de recherche

Laboratoire d'Astrophysique de Bordeaux (LAB) - UMR 5804