{ "id": "1002.1864", "version": "v2", "published": "2010-02-09T19:18:25.000Z", "updated": "2010-03-16T15:52:38.000Z", "title": "The standard model of star formation applied to massive stars: accretion disks and envelopes in molecular lines", "authors": [ "Eric Keto", "Qizhou Zhang" ], "comment": "Accepted MNRAS", "categories": [ "astro-ph.GA" ], "abstract": "We address the question of whether the formation of high-mass stars is similar to or differs from that of solar-mass stars through new molecular line observations and modeling of the accretion flow around the massive protostar IRAS20126+4104. We combine new observations of NH3(1,1) and (2,2) made at the Very Large Array, new observations of CHCN(13-12) made at the Submillimeter Array, previous VLA observations of NH(3,3), NH(4,4), and previous Plateau de Bure observations of C34S(2-1), C34S(5-4), and CHCN(12-11) to obtain a data set of molecular lines covering 15 to 419 K in excitation energy. We compare these observations against simulated molecular line spectra predicted from a model for high-mass star formation based on a scaled-up version of the standard disk-envelope paradigm developed for accretion flows around low-mass stars. We find that in accord with the standard paradigm, the observations require both a warm, dense, rapidly-rotating disk and a cold, diffuse infalling envelope. This study suggests that accretion processes around 10 M stars are similar to those of solar mass stars.", "revisions": [ { "version": "v2", "updated": "2010-03-16T15:52:38.000Z" } ], "analyses": { "keywords": [ "star formation", "accretion disks", "standard model", "massive stars", "observations" ], "tags": [ "journal article" ], "publication": { "doi": "10.1111/j.1365-2966.2010.16672.x", "journal": "Monthly Notices of the Royal Astronomical Society", "year": 2010, "month": "Jul", "volume": 406, "number": 1, "pages": 102 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 845409, "adsabs": "2010MNRAS.406..102K" } } }