TEAGUE, R.,; GUILLOTEAU, S.; SEMENOV, D.,; HENNING, T.,; DUTREY, Anne; PIETU, V.,; BIRNSTIEL, T.,; CHAPILLON, E.; HOLLENBACH, D.,; GORTI, U.,

Métadonnées

Afficher la notice complète

Licence d’utilisation du document

TEAGUE, R.,

GUILLOTEAU, S.
AMOR 2016

SEMENOV, D.,

Langue

Autre document

Ce document a été publié dans

2016-07p. 2016yCat..35920049T

Résumé en anglais

The observations were performed using ALMA on May 13, 2015 under excellent weather conditions (Cycle 2, 2013.1.00387.S). The receivers were tuned to cover CO J=(2-1), CS J=(5-4) and all strong hyperfine components of CN N=(2-1) simultaneously. The correlator was configured to deliver very high spectral resolution, with a channel spacing of 15kHz (and an effective velocity resolution of 40m/s) for the CO J=(2-1) and CS J=(5-4) lines, and 30kHz (80m/s) for the CN N=(2-1) transition.(2 data files).< Réduire

Origine

Importé de hal

Unités de recherche

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