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

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TEAGUE, R.,

GUILLOTEAU, S.
AMOR 2016

SEMENOV, D.,

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2016-07p. 2016yCat..35920049T

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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).< Leer menos

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