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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3T4GBAH
Repositorysid.inpe.br/mtc-m21c/2019/04.08.11.40
Last Update2019:04.08.11.40.37 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2019/04.08.11.40.37
Metadata Last Update2020:01.06.11.42.12 (UTC) administrator
DOI10.1093/mnras/sty3097
ISSN0035-8711
1365-2966
Citation KeyBelloniGieSanAskCie:2019:CaVaPr
TitleMOCCA-SURVEY database I. accreting white dwarf binary systems in globular clusters - IV. cataclysmic variables - properties of bright and faint populations
Year2019
MonthFeb.
Access Date2024, May 17
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size1551 KiB
2. Context
Author1 Belloni, Diogo Teixeira
2 Giersz, Mirek
3 Sandoval, Liliana E. Rivera
4 Askar, Abbas
5 Ciecielag, Pawel
Group1 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Polish Academy of Sciences
3 Texas Tech University
4 Polish Academy of Sciences
5 Polish Academy of Sciences
Author e-Mail Address1 diogo.belloni@inpe.br
2 mig@camk.edu.pl
3 Liliana.Rivera@ttu.edu
JournalMonthly Notices of the Royal Astronomical Society
Volume483
Number1
Pages315-331
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)2019-04-08 11:40:37 :: simone -> administrator ::
2019-04-08 11:40:37 :: administrator -> simone :: 2019
2019-04-08 11:41:14 :: simone -> administrator :: 2019
2020-01-06 11:42:12 :: administrator -> simone :: 2019
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsmethods: numerical
novae
cataclysmic variables
globular clusters: general
binaries: general
AbstractWe investigate here populations of cataclysmic variables (CVs) in a set of 288 globular cluster (GC) models evolved with the MOCCA code. This is by far the largest sample of GC models ever analysed with respect to CVs. Contrary to what has been argued for a long time, we found that dynamical destruction of primordial CV progenitors is much stronger in GCs than dynamical formation of CVs, and that dynamically formed CVs and CVs formed under no/weak influence of dynamics have similar white dwarf mass distributions. In addition, we found that, on average, the detectable CV population is predominantly composed of CVs formed via a typical common envelope phase (CEP) (greater than or similar to 70 per cent), that only approximate to 2-4 per cent of all CVs in a GC are likely to be detectable, and that core-collapsed models tend to have higher fractions of bright CVs than non-core-collapsed ones. We also consistently show, for the first time, that the properties of bright and faint CVs can be understood by means of the pre-CV and CV formation rates, their properties at their formation times and cluster half-mass relaxation times. Finally, we show that models following the initial binary population proposed by Kroupa and set with low CEP efficiency better reproduce the observed amount of CVs and CV candidates in NGC 6397, NGC 6752 and 47 Tuc. To progress with comparisons, the essential next step is to properly characterize the candidates as CVs (e.g. by obtaining orbital periods and mass ratios).
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > MOCCA-SURVEY database I....
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/3T4GBAH
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34R/3T4GBAH
Languageen
Target Filebelloni_mocca.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
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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