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SuperMALT: Physical and Chemical Properties of Massive and Dense Clumps

Authordc.contributor.authorNeupane, Sudeep 
Authordc.contributor.authorGaray Brignardello, Guido 
Authordc.contributor.authorContreras, Yanett 
Cita de ítemdc.identifier.citationProceedings of the International Astronomical Union, Volumen 13, Issue S332, 2017, Pages 254-260
Abstractdc.description.abstractThe SuperMALT survey is observing 76 MALT90 clumps at different evolutionary stages (from pre-stellar or quiescent to HII) in high excitation molecular lines and key isotopomers using the Apex 12m telescope with an angular resolution of ∼20 and a velocity resolution of ∼0.1 km/s. The aim of this survey is to determine the physical, chemical, and kinematical properties of the gas within clumps as they evolve. Here we report some preliminary results based on observations of the J=3-2 & 4-3 lines of HNC, HCN, HCO+, N2H+ and of the J=3-2 line of the isotopologue H13CO+. We find that the morphologies and line profiles vary with the evolutionary stage of the clumps. The average line width increases from quiescent to HII clumps while line ratios show hint of chemical differences among the various evolutionary stages.
Publisherdc.publisherCambridge University Press
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile
Link to Licensedc.rights.uri
Sourcedc.sourceProceedings of the International Astronomical Union
Keywordsdc.subjectISM: clouds
Keywordsdc.subjectISM: evolution
Keywordsdc.subjectISM: molecules
Keywordsdc.subjectline: profiles
Títulodc.titleSuperMALT: Physical and Chemical Properties of Massive and Dense Clumps
Document typedc.typeArtículo de revista
Indexationuchile.indexArtículo de publicación SCOPUS

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Except where otherwise noted, this item's license is described as Attribution-NonCommercial-NoDerivs 3.0 Chile