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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/44KJHES
Repositorysid.inpe.br/mtc-m21c/2021/05.04.13.25   (restricted access)
Last Update2021:11.05.13.45.10 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2021/05.04.13.25.49
Metadata Last Update2022:04.03.19.24.41 (UTC) administrator
ISSN1824-8039
Citation KeyBelloniRive:2021:PrCaVa
TitleProperties of cataclysmic variables in globular clusters
Year2021
MonthFeb.
Access Date2024, Apr. 25
Type of Workconference paper
Secondary TypePRE PI
Number of Files1
Size504 KiB
2. Context
Author1 Belloni, Diogo Teixeira
2 Rivera Sandoval, Liliana
Group1 DIAST-CGCE-INPE-MCTI-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 diogo.belloni@inpe.br
2 Liliana.Rivera@ttu.edu
JournalProceedings of Science
Volume368
Pagese013
Secondary MarkB4_ENGENHARIAS_III C_ASTRONOMIA_/_FÍSICA
History (UTC)2021-06-23 13:33:17 :: simone -> administrator :: 2021
2021-07-02 02:27:15 :: administrator -> simone :: 2021
2021-11-05 13:45:10 :: simone -> administrator :: 2021
2022-04-03 19:24:41 :: administrator -> simone :: 2021
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractThe study of star clusters plays an important role in our understanding of the Universe since these systems are natural laboratories for testing theories of stellar dynamics and evolution. Particularly, globular clusters (GCs) are one of the most important objects for studying the formation and the physical nature of exotic systems which in turn provide basic information and tools that can help us to understand the formation and evolution processes of star clusters themselves, galaxies and, in general, the young Universe. Among the most interesting objects in GCs are the cataclysmic variables (CVs), which are interacting binaries harbouring a white dwarf accreting from a low-mass companion. Since GC densities are sufficiently high that dynamical encounters involving binaries should be common, CV progenitors are expected to be affected by dynamics in some way in the early stages. In this article we review the formation channels and the influence of dynamics on the CV population in GCs. In particular, we review recent progress in numerical simulations. Furthermore, we discuss observational properties of CVs in GCs and the techniques used to identify and study them. We focus the discussion on the multi-wavelength observations carried out with HST and Chandra on the best-studied GCs NGC 6397, NGC 6752, 47 Tucanae and ω Centauri; on the recent spectroscopic findings with MUSE, and on updates regarding the correlation between the number of faint X-ray sources and the cluster stellar encounter rate. Finally, we discuss some observational prospects that might potentially help future investigations.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Properties of cataclysmic...
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Languageen
Target Filebelloni_properties.pdf
User Groupsimone
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Visibilityshown
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
Citing Item Listsid.inpe.br/bibdigital@80/2006/04.07.15.50.13 1
DisseminationPORTALCAPES; SCOPUS.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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