FAVRE, C.; FEDELE, D.; SEMENOV, D.; PARFENOV, S.; CODELLA, C.; CECCARELLI, C.; BERGIN, E. A.; CHAPILLON, E.; TESTI, L.; HERSANT, F.; LEFLOCH, B.; FONTANI, F.; BLAKE, G. A.; CLEEVES, L. I.; QI, C.; SCHWARZ, K. R.; TAQUET, V.

Métadonnées

Afficher la notice complète

Licence d’utilisation du document

Langue

Autre document

Ce document a été publié dans

2019

Résumé en anglais

The observations were performed toward TW Hya on 2016 May 31 and on 2016 June 1 with 39 antennas and baselines from 15.1m (6.5kλ) up to 713.1m (310.0kλ) with an on-source time of about 39 min with ALMA during Cycle 3. The spectral setup consisted of (i) six spectral windows, each with 960 channels and a channel width used during the observations of 244.141kHz (about 0.6km/s) that covered about 1.4GHz between 129.538 and 132.405GHz, and (ii) one spectral window, centered at 130.973GHz, of 2GHz bandwidth (128 channels each of 15.625MHz) for continuum imaging. (2 data files).< Réduire

Mots clés en anglais

Molecular data

Interstellar medium

YSOs

Radio continuum

Origine

Importé de hal

Unités de recherche

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