MALT90: The Millimetre Astronomy Legacy Team 90 GHz Survey
dc.contributor.author | JACKSON, J. M. | |
dc.contributor.author | RATHBORNE, J. M. | |
dc.contributor.author | FOSTER, J. B. | |
dc.contributor.author | WHITAKER, J. S. | |
dc.contributor.author | SANHUEZA, P. | |
dc.contributor.author | CLAYSMITH, C. | |
dc.contributor.author | MASCOOP, J. L. | |
hal.structure.identifier | Max-Planck-Institut für Radioastronomie [MPIFR] | |
dc.contributor.author | WIENEN, M. | |
dc.contributor.author | BREEN, S. L. | |
hal.structure.identifier | FORMATION STELLAIRE 2013 | |
dc.contributor.author | HERPIN, Fabrice | |
hal.structure.identifier | FORMATION STELLAIRE 2013 | |
dc.contributor.author | DUARTE-CABRAL, A. | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | CSENGERI, T. | |
hal.structure.identifier | Swinburne University of Technology (Hawthorn campus) | |
dc.contributor.author | LONGMORE, S. | |
hal.structure.identifier | Max-Planck-Institut für Radioastronomie [MPIFR] | |
dc.contributor.author | CONTRERAS, Y. | |
dc.contributor.author | INDERMUEHLE, B. | |
dc.contributor.author | BARNES, P. J. | |
hal.structure.identifier | Laboratoire de Probabilités et Modèles Aléatoires [LPMA] | |
dc.contributor.author | WALSH, A. J. | |
dc.contributor.author | CUNNINGHAM, M. R. | |
dc.contributor.author | BROOKS, K. J. | |
dc.contributor.author | BRITTON, T. R. | |
hal.structure.identifier | Australia Telescope National Facility [ATNF] | |
dc.contributor.author | VORONKOV, M. A. | |
dc.contributor.author | URQUHART, J. S. | |
hal.structure.identifier | Instituto Dom Luiz | |
dc.contributor.author | ALVES, J. | |
dc.contributor.author | JORDAN, C. H. | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | HILL, T. | |
dc.contributor.author | HOQ, S. | |
dc.contributor.author | FINN, S. | |
dc.contributor.author | C., S. | |
hal.structure.identifier | Swinburne University of Technology (Hawthorn campus) | |
dc.contributor.author | BAINS, I. | |
hal.structure.identifier | FORMATION STELLAIRE 2013 | |
dc.contributor.author | BONTEMPS, Sylvain | |
hal.structure.identifier | Departamento de Astronomia [DAS] | |
dc.contributor.author | BRONFMAN, L. | |
dc.contributor.author | CASWELL, J. L. | |
dc.contributor.author | DEHARVENG, L. | |
dc.contributor.author | ELLINGSEN, S. P. | |
dc.contributor.author | FULLER, G. A. | |
dc.contributor.author | GARAY, G. | |
dc.contributor.author | GREEN, J. A. | |
dc.contributor.author | HINDSON, L. | |
dc.contributor.author | JONES, P. A. | |
dc.contributor.author | LENFESTEY, C. | |
dc.contributor.author | LO, N. | |
dc.contributor.author | LOWE, V. | |
dc.contributor.author | MARDONES, D. | |
hal.structure.identifier | Max-Planck-Institut für Radioastronomie [MPIFR] | |
dc.contributor.author | MENTEN, K. M. | |
hal.structure.identifier | Institut de Recherches sur les lois Fondamentales de l'Univers [IRFU] | |
dc.contributor.author | MINIER, V. | |
dc.contributor.author | MORGAN, L. K. | |
hal.structure.identifier | Institut de Recherches sur les lois Fondamentales de l'Univers [IRFU] | |
dc.contributor.author | MOTTE, F. | |
hal.structure.identifier | German Aerospace Center [DLR] | |
dc.contributor.author | MULLER, E. | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | PERETTO, N. | |
hal.structure.identifier | Swinburne University of Technology (Hawthorn campus) | |
dc.contributor.author | PURCELL, C. R. | |
hal.structure.identifier | Max Planck Institute for Radio Astronomy | |
hal.structure.identifier | I. Physikalisches Institut [Köln] | |
dc.contributor.author | SCHILKE, P. | |
hal.structure.identifier | FORMATION STELLAIRE 2013 | |
dc.contributor.author | SCHNEIDER, N. | |
hal.structure.identifier | Max-Planck-Institut für Radioastronomie [MPIFR] | |
dc.contributor.author | SCHULLER, F. | |
dc.contributor.author | TITMARSH, A. | |
hal.structure.identifier | Max-Planck-Institut für Radioastronomie [MPIFR] | |
dc.contributor.author | WYROWSKI, F. | |
dc.contributor.author | ZAVAGNO, Annie | |
dc.date.created | 2013-10-03 | |
dc.date.issued | 2013 | |
dc.identifier.issn | 1323-3580 | |
dc.description.abstractEn | The Millimetre Astronomy Legacy Team 90 GHz (MALT90) survey aims to characterise the physical and chemical evolution of high-mass star-forming clumps. Exploiting the unique broad frequency range and on-the-fly mapping capabilities of the Australia Telescope National Facility Mopra 22 m single-dish telescope, MALT90 has obtained 3' x 3' maps toward ~2000 dense molecular clumps identified in the ATLASGAL 870 um Galactic plane survey. The clumps were selected to host the early stages of high-mass star formation and to span the complete range in their evolutionary states (from prestellar, to protostellar, and on to HII regions and photodissociation regions). Because MALT90 mapped 16 lines simultaneously with excellent spatial (38") and spectral (0.11 km/s) resolution, the data reveal a wealth of information about the clump's morphologies, chemistry, and kinematics. In this paper we outline the survey strategy, observing mode, data reduction procedure, and highlight some early science results. All MALT90 raw and processed data products are available to the community. With its unprecedented large sample of clumps, MALT90 is the largest survey of its type ever conducted and an excellent resource for identifying interesting candidates for high resolution studies with ALMA. | |
dc.language.iso | en | |
dc.publisher | Cambridge University Press (CUP) | |
dc.subject.en | Astrophysics | |
dc.subject.en | Galaxy Astrophysics | |
dc.title.en | MALT90: The Millimetre Astronomy Legacy Team 90 GHz Survey | |
dc.type | Article de revue | |
dc.identifier.doi | 10.1017/pasa.2013.37 | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR] | |
dc.subject.hal | Physique [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR] | |
dc.identifier.arxiv | 1310.1131 | |
bordeaux.journal | Publications of the Astronomical Society of Australia | |
bordeaux.page | id.e057 | |
bordeaux.volume | 30 | |
bordeaux.peerReviewed | oui | |
hal.identifier | hal-00870732 | |
hal.version | 1 | |
hal.popular | non | |
hal.audience | Internationale | |
hal.origin.link | https://hal.archives-ouvertes.fr//hal-00870732v1 | |
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