Radiation-hydrodynamic simulations of massive star formation with protostellar outflows
dc.contributor.author | Cunningham, Andrew J. | |
dc.contributor.author | Klein, Richard I. | |
dc.contributor.author | Krumholz, Mark | |
dc.contributor.author | McKee, Christopher F. | |
dc.date.accessioned | 2018-11-29T22:52:20Z | |
dc.date.available | 2018-11-29T22:52:20Z | |
dc.date.issued | 2011 | |
dc.date.updated | 2018-11-29T07:45:06Z | |
dc.format.mimetype | application/pdf | en_AU |
dc.identifier.issn | 0004-637X | |
dc.identifier.uri | http://hdl.handle.net/1885/152137 | |
dc.publisher | IOP Publishing | |
dc.source | The Astrophysical Journal | |
dc.subject | Keywords: binaries: general; stars: formation; stars: pre-main sequence; stars: winds, outflows | |
dc.title | Radiation-hydrodynamic simulations of massive star formation with protostellar outflows | |
dc.type | Journal article | |
dcterms.accessRights | Open Access | en_AU |
local.bibliographicCitation.issue | 2 | |
local.contributor.affiliation | Cunningham, Andrew J., Lawrence Livermore National Laboratory | |
local.contributor.affiliation | Klein, Richard I., Lawrence Livermore National Laboratory | |
local.contributor.affiliation | Krumholz, Mark, College of Science, ANU | |
local.contributor.affiliation | McKee, Christopher F., University of California | |
local.contributor.authoremail | u1000557@anu.edu.au | |
local.contributor.authoruid | Krumholz, Mark, u1000557 | |
local.description.notes | Imported from ARIES | |
local.identifier.absfor | 020103 - Cosmology and Extragalactic Astronomy | |
local.identifier.absfor | 020104 - Galactic Astronomy | |
local.identifier.absseo | 970102 - Expanding Knowledge in the Physical Sciences | |
local.identifier.ariespublication | a383154xPUB3447 | |
local.identifier.citationvolume | 740 | |
local.identifier.doi | 10.1088/0004-637X/740/2/107 | |
local.identifier.scopusID | 2-s2.0-80053952310 | |
local.identifier.thomsonID | 000296762900057 | |
local.identifier.uidSubmittedBy | a383154 | |
local.type.status | Published Version |
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