CSENGERI, T.; BONTEMPS, Sylvain; WYROWSKI, F.; BELLOCHE, A.; MENTEN, K. M.; LEURINI, S.; BEUTHER, H.; BRONFMAN, L.; COMMERCON, B.; CHAPILLON, E.; LONGMORE, S.; PALAU, A.; TAN, J. C.; URQUHART, J. S.

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CSENGERI, T.
Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]

BONTEMPS, Sylvain
FORMATION STELLAIRE 2018

WYROWSKI, F.
Max-Planck-Institut für Radioastronomie [MPIFR]

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2018

Résumé en anglais

These are the corresponding continuum data published in the paper. G328.2551-0.5321 has been observed with ALMA in Cycle 2, and the phase center was (RA,DE)J2000=(15:58:00.05, -53:57:57.8). We used 11 of the 7m antennas on the 2014 July 8 and 16, as well as 34 and 35 of the 12m antennas on 2015 May 3, and 2015 September 1, respectively. The 7m array observations are discussed in detail in Csengeri et al. (2017, Cat. J/A+A/600/L10). Here we also present the 12m array observations, for which the baseline range is 15m (17kλ) to 1574m (1809kλ). The total time on source was 7.4 minutes, and the system temperature (Tsys) varies between 120 and 200K. (2 data files).< Réduire

Mots clés en italien

Radio sources

YSOs

Interstellar medium

Origine

Importé de hal

Unités de recherche

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