1. Identity statement | |
Reference Type | Journal Article |
Site | mtc-m16d.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 8JMKD3MGP7W/37JTSB8 |
Repository | sid.inpe.br/mtc-m19@80/2010/06.01.17.25 (restricted access) |
Last Update | 2010:06.01.17.25.54 (UTC) administrator |
Metadata Repository | sid.inpe.br/mtc-m19@80/2010/06.01.17.25.56 |
Metadata Last Update | 2018:06.05.04.36.42 (UTC) administrator |
Secondary Key | INPE--PRE/ |
DOI | 10.1016/j.asr.2010.03.009 |
ISSN | 0273-1177 |
Citation Key | ShuLuHaChChWu:2010:EvGlCl |
Title | The evolution of globular clusters |
Year | 2010 |
Month | Aug. |
Access Date | 2024, Apr. 28 |
Secondary Type | PRE PI |
Number of Files | 1 |
Size | 508 KiB |
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2. Context | |
Author | 1 Shu, Chenggang 2 Luo, Zhijian 3 Han, Mao-an 4 Chian, Abraham C. -L. 5 Chen, Wen-Ping 6 Wu, Zhen-yu |
Group | 1 DGE-CEA-INPE-MCT-BR |
Affiliation | 1 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 |
Journal | Advances in Space Research |
Volume | 46 |
Number | 4 |
Pages | 500-508. |
Secondary Mark | B4_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 |
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3. Content and structure | |
Is the master or a copy? | is the master |
Content Stage | completed |
Transferable | 1 |
Content Type | External Contribution |
Version Type | publisher |
Keywords | Globular clusters Evolution Dynamics |
Abstract | Taking 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. |
Area | CEA |
Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > The evolution of... |
doc Directory Content | access |
source Directory Content | there are no files |
agreement Directory Content | there are no files |
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4. Conditions of access and use | |
Language | en |
Target File | the evolution of globular.pdf |
User Group | administrator banon marciana simone |
Visibility | shown |
Archiving Policy | denypublisher denyfinaldraft24 |
Read Permission | deny from all and allow from 150.163 |
Update Permission | not transferred |
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5. Allied materials | |
Mirror Repository | sid.inpe.br/mtc-m19@80/2009/08.21.17.02.53 |
Next Higher Units | 8JMKD3MGPCW/3EU29DP |
Dissemination | WEBSCI; PORTALCAPES; MGA; COMPENDEX. |
Host Collection | sid.inpe.br/mtc-m19@80/2009/08.21.17.02 |
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6. Notes | |
Empty Fields | alternatejournal 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 |
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7. Description control | |
e-Mail (login) | marciana |
update | |
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