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1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Sitemtc-m21c.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34R/44D5FPS
Repositóriosid.inpe.br/mtc-m21c/2021/03.25.16.16
Repositório de Metadadossid.inpe.br/mtc-m21c/2021/03.25.16.16.31
Última Atualização dos Metadados2022:04.03.19.25.17 (UTC) administrator
Chave SecundáriaINPE--PRE/
Chave de CitaçãoSouzaOlivRodrLima:2021:SpAnMC
TítuloSpectroscopic analysis of the mCV candidate CSS0357+10 with SOAR Telescope data
Ano2021
Data de Acesso09 maio 2024
Tipo SecundárioPRE CN
2. Contextualização
Autor1 Souza, D. C.
2 Oliveira, A. S.
3 Rodrigues, Cláudia Vilega
4 Lima, Isabel de Jesus
Identificador de Curriculo1
2
3 8JMKD3MGP5W/3C9JGS5
Grupo1
2
3 DIAST-CGCE-INPE-MCTI-GOV-BR
4 AST-CEA-DIPGR-INPE-MCTI-GOV-BR
Afiliação1 Universidade do Vale do Paraíba (UNIVAP)
2 Universidade do Vale do Paraíba (UNIVAP)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1
2
3 claudia.vilega@gmail.com
4 isabellima01@gmail.com
Nome do EventoSimpósio Brasileiro de Geofísica Espacial e Aeronomia, 8 (SBGEA)
Localização do EventoOnline
Data22-26 mar.
Histórico (UTC)2021-03-25 16:16:31 :: simone -> administrator ::
2022-04-03 19:25:17 :: administrator -> simone :: 2021
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
ResumoCataclysmic variables are binary systems where the primary component is a white dwarf star and the secondary is a main sequence star, usually a red dwarf. Due to the proximity of the system components the secondary star fills its Roche lobe causing a flow of ionized gas expelled by the internal Lagrange point forming an accretion disk around the primary. Some of these white dwarfs may have a magnetic field strong enough to change the path of the gas causing it to follow the lines of its field to form an accretion column that collides with the white dwarf near its magnetic pole instead of form a disc. In others the disk is partially formed with its internal part following the magnetic field. The first is known as polar and the second as intermediate polar (IPs), both are types of magnetic cataclysmic variables (mCVs). In our project to search and characterize new mCVs several candidates are selected from the Catalina Real Time Transient photometric survey (CRTS) to confirm whether the system belongs to this class. Several systems have already been confirmed as mCV. Among them CSS 0357+10 which had also been identified as an x-ray source was chosen for a more detailed study. In this work the analysis of the spectrum of this system obtained in the SOAR telescope was performed. The spectrum is dominated by hydrogen emission lines in the Balmer series and He II ionization characteristic, properties of a mCV spectrum.
ÁreaCEA
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4. Condições de acesso e uso
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Grupo de Usuáriossimone
Visibilidadeshown
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3F2NE4L
8JMKD3MGPCW/46KTFK8
Acervo Hospedeirourlib.net/www/2017/11.22.19.04
6. Notas
Campos Vaziosarchivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn keywords label lineage mark mirrorrepository nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup readpermission rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume
7. Controle da descrição
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