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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3TKBH45
Repositorysid.inpe.br/mtc-m21c/2019/07.08.15.50
Last Update2019:07.08.15.50.29 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2019/07.08.15.50.29
Metadata Last Update2020:01.06.11.42.16 (UTC) administrator
DOI10.1093/mnras/stz1187
ISSN0035-8711
1365-2966
Citation KeySartorioVanFalWooNet:2019:EfPhFe
TitleMassive star formation via torus accretion: the effect of photoionization feedback
Year2019
MonthJuly
Access Date2024, May 16
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size3520 KiB
2. Context
Author1 Sartorio, Nina Sanches
2 Vandenbroucke, B.
3 Falceta-Gonçalves, Diego
4 Wood, K.
5 Neto, E.
ORCID1
2 0000-0001-7241-1704
Group1 AST-CEA-SESPG-INPE-MCTIC-GOV-BR
2
3 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 University of St Andrews
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 University of St Andrews
5 Harvard-Smithsonian Center for Astrophysics
Author e-Mail Address1 sartorio.nina@gmail.com
JournalMonthly Notices of the Royal Astronomical Society
Volume486
Number4
Pages5171-5183
Secondary MarkA1_QUÍMICA A1_INTERDISCIPLINAR A1_GEOCIÊNCIAS A1_ENGENHARIAS_III A2_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA A2_ASTRONOMIA_/_FÍSICA B2_ENSINO B5_ENGENHARIAS_IV
History (UTC)2019-07-08 15:50:29 :: simone -> administrator ::
2019-07-08 15:50:30 :: administrator -> simone :: 2019
2019-07-08 15:51:12 :: simone -> administrator :: 2019
2020-01-06 11:42:16 :: administrator -> simone :: 2019
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsradiative transfer
methods: numerical
stars: massive
H II regions
accretion discs
AbstractThe formation of massive stars is a longstanding problem. Although a number of theories of massive star formation exist, ideas appear to converge to a disc-mediated accretion scenario. Here, we present radiative hydrodynamic simulations of a star-accreting mass via a disc embedded in a torus. We use a Monte Carlo based radiation hydrodynamics code to investigate the impact that ionizing radiation has on the torus. Ionized regions in the torus midplane are found to be either gravitationally trapped or in pressure-driven expansion depending on whether or not the size of the ionized region exceeds a critical radius. Trapped H II regions in the torus plane allow accretion to progress, while expanding H II regions disrupt the accretion torus preventing the central star from aggregating more mass, thereby setting the stars final mass. We obtain constraints for the luminosities and torus densities that lead to both scenarios.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Massive star formation...
Arrangement 2urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > AST > Massive star formation...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34R/3TKBH45
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34R/3TKBH45
Languageen
Target Filesartorio.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
8JMKD3MGPCW/3F2NE4L
Citing Item Listsid.inpe.br/bibdigital/2013/10.01.00.07 4
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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