VizieR Online Data Catalog: G328.2551-0.5321 ALMA images (Csengeri+, 2018)
| hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
| dc.contributor.author | CSENGERI, T. | |
| hal.structure.identifier | FORMATION STELLAIRE 2018 | |
| dc.contributor.author | BONTEMPS, Sylvain | |
| hal.structure.identifier | Max-Planck-Institut für Radioastronomie [MPIFR] | |
| dc.contributor.author | WYROWSKI, F. | |
| hal.structure.identifier | Max-Planck-Institut für Radioastronomie [MPIFR] | |
| dc.contributor.author | BELLOCHE, A. | |
| hal.structure.identifier | Max-Planck-Institut für Radioastronomie [MPIFR] | |
| dc.contributor.author | MENTEN, K. M. | |
| hal.structure.identifier | Max-Planck-Institut für Radioastronomie [MPIFR] | |
| dc.contributor.author | LEURINI, S. | |
| hal.structure.identifier | Max-Planck-Institut für Astronomie [MPIA] | |
| dc.contributor.author | BEUTHER, H. | |
| hal.structure.identifier | Departamento de Astronomia [DAS] | |
| dc.contributor.author | BRONFMAN, L. | |
| hal.structure.identifier | Centre de Recherche Astrophysique de Lyon [CRAL] | |
| dc.contributor.author | COMMERCON, B. | |
| hal.structure.identifier | AMOR 2018 | |
| dc.contributor.author | CHAPILLON, E. | |
| hal.structure.identifier | Swinburne University of Technology (Hawthorn campus) | |
| dc.contributor.author | LONGMORE, S. | |
| dc.contributor.author | PALAU, A. | |
| hal.structure.identifier | University of Florida [Gainesville] [UF] | |
| dc.contributor.author | TAN, J. C. | |
| hal.structure.identifier | School of Physical Sciences, University of Kent | |
| dc.contributor.author | URQUHART, J. S. | |
| dc.date.issued | 2018 | |
| dc.description | VizieR On-line Data Catalog: J/A+A/617/A89. Originally published in: 2018A&A...617A..89C | |
| dc.description.abstractEn | 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). | |
| dc.language.iso | it | |
| dc.type | Autre document | |
| dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique galactique [astro-ph.GA] | |
| dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO] | |
| hal.identifier | hal-01901661 | |
| hal.version | 1 | |
| hal.popular | non | |
| dc.subject.it | Radio sources | |
| dc.subject.it | YSOs | |
| dc.subject.it | Interstellar medium | |
| dc.title.it | VizieR Online Data Catalog: G328.2551-0.5321 ALMA images (Csengeri+, 2018) | |
| hal.origin.link | https://hal.archives-ouvertes.fr//hal-01901661v1 | |
| bordeaux.COinS | ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2018&rft.au=CSENGERI,%20T.&BONTEMPS,%20Sylvain&WYROWSKI,%20F.&BELLOCHE,%20A.&MENTEN,%20K.%20M.&rft.genre=unknown |
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