dc.creatorGaray Brignardello, Guido
dc.creatorFaúndez, Santiago
dc.creatorMardones Pérez, Diego
dc.creatorBronfman Aguiló, Leonardo
dc.date.accessioned2013-01-15T20:26:16Z
dc.date.available2013-01-15T20:26:16Z
dc.date.created2013-01-15T20:26:16Z
dc.date.issued2004-07-20
dc.identifierASTROPHYSICAL JOURNAL Volume: 610 Issue: 1 Pages: 313-319 Part: Part 1 Published: JUL 20 2004
dc.identifier0004-637X
dc.identifierDOI: 10.1086/421437
dc.identifierhttps://repositorio.uchile.cl/handle/2250/125758
dc.description.abstractWe report the identification, from a 1.2 mm dust continuum emission survey toward massive star-forming regions, of four strong 1.2 mm sources without counterparts at mid-infrared (Midcourse Space Experiment [MSX]) and far-infrared (IRAS) wavelengths. They have radii in the range 0.2-0.3 pc, dust temperatures less than or equal to17 K, masses in the range 4 x 10(2)-2 x 10(3) M-circle dot, and densities of similar to2 x 10(5) cm(-3). We suggest that these objects are massive and dense cold cores that will eventually collapse to form high-mass stars.
dc.languageen
dc.publisherUNIV CHICAGO PRESS
dc.subjectdust, extinction
dc.titleDiscovery of four new massive and dense cold cores
dc.typeArtículo de revista


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