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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/37JTSB8
Repositorysid.inpe.br/mtc-m19@80/2010/06.01.17.25   (restricted access)
Last Update2010:06.01.17.25.54 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19@80/2010/06.01.17.25.56
Metadata Last Update2018:06.05.04.36.42 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1016/j.asr.2010.03.009
ISSN0273-1177
Citation KeyShuLuHaChChWu:2010:EvGlCl
TitleThe evolution of globular clusters
Year2010
MonthAug.
Access Date2024, Apr. 28
Secondary TypePRE PI
Number of Files1
Size508 KiB
2. Context
Author1 Shu, Chenggang
2 Luo, Zhijian
3 Han, Mao-an
4 Chian, Abraham C. -L.
5 Chen, Wen-Ping
6 Wu, Zhen-yu
Group1 DGE-CEA-INPE-MCT-BR
Affiliation1 Shanghai Normal University
2 Shanghai Normal University
3 Shanghai Normal University
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 National Central University
6 Chinese Academy of Sciences
JournalAdvances in Space Research
Volume46
Number4
Pages500-508.
Secondary MarkB4_ASTRONOMIA_/_FÍSICA B3_CIÊNCIAS_BIOLÓGICAS_I B1_ENGENHARIAS_III B1_ENGENHARIAS_IV B1_GEOCIÊNCIAS B1_INTERDISCIPLINAR
History (UTC)2010-07-05 14:54:46 :: simone -> marciana :: 2010
2012-01-26 11:29:11 :: marciana -> administrator :: 2010
2012-07-15 03:41:32 :: administrator -> banon :: 2010
2013-02-19 13:54:26 :: banon -> administrator :: 2010
2018-06-05 04:36:42 :: administrator -> marciana :: 2010
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsGlobular clusters
Evolution
Dynamics
AbstractTaking a wide range of the initial conditions, including spatial density distribution and mass function etc, the dynamical evolution of globular clusters in the Milky Way is investigated in detail by means of Monte Carlo simulations. Four dynamic mechanisms are considered: stellar evaporation, stellar evolution, tidal shocks due to both the disk and bulge, and dynamical friction. It is found that stellar evaporation dominates the evolution of low-mass clusters and all four are important for massive ones. For both the power-law and lognormal initial clusters mass functions, we can find the best-fit models which can match the present-day observations with their main features of the mass function almost unchanged after evolution of several Gyr. This implies that it is not possible to determine the initial mass function only based on the observed ones today. Moreover, the dispersion of the modelled mass functions mainly depends on the potential wells of host galaxies with the almost constant peaks, which is consistent with current observations.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > The evolution of...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target Filethe evolution of globular.pdf
User Groupadministrator
banon
marciana
simone
Visibilityshown
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Mirror Repositorysid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Next Higher Units8JMKD3MGPCW/3EU29DP
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress electronicmailaddress format isbn label lineage mark nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url
7. Description control
e-Mail (login)marciana
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