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dc.contributor.authorJACKSON, J. M.
dc.contributor.authorRATHBORNE, J. M.
dc.contributor.authorFOSTER, J. B.
dc.contributor.authorWHITAKER, J. S.
dc.contributor.authorSANHUEZA, P.
dc.contributor.authorCLAYSMITH, C.
dc.contributor.authorMASCOOP, J. L.
hal.structure.identifierMax-Planck-Institut für Radioastronomie [MPIFR]
dc.contributor.authorWIENEN, M.
dc.contributor.authorBREEN, S. L.
hal.structure.identifierFORMATION STELLAIRE 2013
dc.contributor.authorHERPIN, Fabrice
hal.structure.identifierFORMATION STELLAIRE 2013
dc.contributor.authorDUARTE-CABRAL, A.
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorCSENGERI, T.
hal.structure.identifierSwinburne University of Technology (Hawthorn campus)
dc.contributor.authorLONGMORE, S.
hal.structure.identifierMax-Planck-Institut für Radioastronomie [MPIFR]
dc.contributor.authorCONTRERAS, Y.
dc.contributor.authorINDERMUEHLE, B.
dc.contributor.authorBARNES, P. J.
hal.structure.identifierLaboratoire de Probabilités et Modèles Aléatoires [LPMA]
dc.contributor.authorWALSH, A. J.
dc.contributor.authorCUNNINGHAM, M. R.
dc.contributor.authorBROOKS, K. J.
dc.contributor.authorBRITTON, T. R.
hal.structure.identifierAustralia Telescope National Facility [ATNF]
dc.contributor.authorVORONKOV, M. A.
dc.contributor.authorURQUHART, J. S.
hal.structure.identifierInstituto Dom Luiz
dc.contributor.authorALVES, J.
dc.contributor.authorJORDAN, C. H.
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorHILL, T.
dc.contributor.authorHOQ, S.
dc.contributor.authorFINN, S.
dc.contributor.authorC., S.
hal.structure.identifierSwinburne University of Technology (Hawthorn campus)
dc.contributor.authorBAINS, I.
hal.structure.identifierFORMATION STELLAIRE 2013
dc.contributor.authorBONTEMPS, Sylvain
hal.structure.identifierDepartamento de Astronomia [DAS]
dc.contributor.authorBRONFMAN, L.
dc.contributor.authorCASWELL, J. L.
dc.contributor.authorDEHARVENG, L.
dc.contributor.authorELLINGSEN, S. P.
dc.contributor.authorFULLER, G. A.
dc.contributor.authorGARAY, G.
dc.contributor.authorGREEN, J. A.
dc.contributor.authorHINDSON, L.
dc.contributor.authorJONES, P. A.
dc.contributor.authorLENFESTEY, C.
dc.contributor.authorLO, N.
dc.contributor.authorLOWE, V.
dc.contributor.authorMARDONES, D.
hal.structure.identifierMax-Planck-Institut für Radioastronomie [MPIFR]
dc.contributor.authorMENTEN, K. M.
hal.structure.identifierInstitut de Recherches sur les lois Fondamentales de l'Univers [IRFU]
dc.contributor.authorMINIER, V.
dc.contributor.authorMORGAN, L. K.
hal.structure.identifierInstitut de Recherches sur les lois Fondamentales de l'Univers [IRFU]
dc.contributor.authorMOTTE, F.
hal.structure.identifierGerman Aerospace Center [DLR]
dc.contributor.authorMULLER, E.
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorPERETTO, N.
hal.structure.identifierSwinburne University of Technology (Hawthorn campus)
dc.contributor.authorPURCELL, C. R.
hal.structure.identifierMax Planck Institute for Radio Astronomy
hal.structure.identifierI. Physikalisches Institut [Köln]
dc.contributor.authorSCHILKE, P.
hal.structure.identifierFORMATION STELLAIRE 2013
dc.contributor.authorSCHNEIDER, N.
hal.structure.identifierMax-Planck-Institut für Radioastronomie [MPIFR]
dc.contributor.authorSCHULLER, F.
dc.contributor.authorTITMARSH, A.
hal.structure.identifierMax-Planck-Institut für Radioastronomie [MPIFR]
dc.contributor.authorWYROWSKI, F.
dc.contributor.authorZAVAGNO, Annie
dc.date.created2013-10-03
dc.date.issued2013
dc.identifier.issn1323-3580
dc.description.abstractEnThe 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.isoen
dc.publisherCambridge University Press (CUP)
dc.subject.enAstrophysics
dc.subject.enGalaxy Astrophysics
dc.title.enMALT90: The Millimetre Astronomy Legacy Team 90 GHz Survey
dc.typeArticle de revue
dc.identifier.doi10.1017/pasa.2013.37
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
dc.identifier.arxiv1310.1131
bordeaux.journalPublications of the Astronomical Society of Australia
bordeaux.pageid.e057
bordeaux.volume30
bordeaux.peerReviewedoui
hal.identifierhal-00870732
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00870732v1
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