Fechar

1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m21c.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34R/43QPQBB
Repositóriosid.inpe.br/mtc-m21c/2020/12.21.10.27   (acesso restrito)
Última Atualização2020:12.21.10.27.29 (UTC) simone
Repositório de Metadadossid.inpe.br/mtc-m21c/2020/12.21.10.27.29
Última Atualização dos Metadados2021:01.08.15.17.20 (UTC) administrator
ISSN1824-8039
Chave de CitaçãoBelloniSand:2020:PrCaVa
TítuloProperties of Cataclysmic Variables in Globular Clusters
Ano2020
Data de Acesso12 maio 2024
Tipo de Trabalhoconference paper
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho504 KiB
2. Contextualização
Autor1 Belloni, Diogo Teixeira
2 Sandoval, Liliana E. Rivera
Grupo1 AST-CEA-SESPG-INPE-MCTIC-GOV-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Texas Tech University
Endereço de e-Mail do Autor1 diogo.belloni@inpe.br
2 Liliana.Rivera@ttu.edu
RevistaProceedings of Science
Volume2020
Histórico (UTC)2020-12-21 10:27:44 :: simone -> administrator :: 2020
2021-01-08 15:17:20 :: administrator -> simone :: 2020
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Tipo de Versãopublisher
ResumoThe 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 harboring 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 Omega 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.
ÁreaCEA
Arranjourlib.net > BDMCI > Fonds > Produção pgr ATUAIS > AST > Properties of Cataclysmic...
Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreement
agreement.html 21/12/2020 07:27 1.0 KiB 
4. Condições de acesso e uso
Idiomaen
Arquivo Alvobelloni_properties.pdf
Grupo de Usuáriossimone
Grupo de Leitoresadministrator
simone
Visibilidadeshown
Permissão de Leituradeny from all and allow from 150.163
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Repositório Espelhourlib.net/www/2017/11.22.19.04.03
Unidades Imediatamente Superiores8JMKD3MGPCW/3F2NE4L
Lista de Itens Citandosid.inpe.br/bibdigital/2013/10.12.16.06 2
DivulgaçãoPORTALCAPES; SCOPUS.
Acervo Hospedeirourlib.net/www/2017/11.22.19.04
6. Notas
NotasThe Golden Age of Cataclysmic Variables and Related Objects, 5., 2019
2–7 Sept. 2019, Palermo, Italy.
Campos Vaziosalternatejournal archivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel doi e-mailaddress format isbn keywords label lineage mark month nextedition number orcid pages parameterlist parentrepositories previousedition previouslowerunit progress project resumeid rightsholder schedulinginformation secondarydate secondarykey secondarymark session shorttitle sponsor subject tertiarymark tertiarytype url
7. Controle da descrição
e-Mail (login)simone
atualizar 


Fechar