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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/3AT7M2S
Repositorysid.inpe.br/mtc-m19/2011/12.02.17.01
Last Update2011:12.02.17.03.05 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19/2011/12.02.17.01.43
Metadata Last Update2018:06.05.04.25.06 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeySilvaRodrCost:2011:PhEfXr
TitlePhase-dependent effects on X-ray spectra of magnetic cataclysmic variables
FormatOn-line
ProjectFAPESP (Proc. 2008/09619-5 and Proc. 2010/06096-1) and CNPq (Proc. 308005/2009-0 - CVR).
Year2011
Access Date2024, May 01
Secondary TypePRE CI
Number of Files1
Size258 KiB
2. Context
Author1 Silva, Karleyne M. G
2 Rodrigues, Claudia Vilega
3 Costa, Joaquim Eduardo Rezende
Resume Identifier1
2 8JMKD3MGP5W/3C9JGS5
3 8JMKD3MGP5W/3C9JHF8
Group1 DAS-CEA-INPE-MCT-BR
2 DAS-CEA-INPE-MCT-BR
3 DAS-CEA-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
e-Mail Addresstereza@sid.inpe.br
Conference NameThe X-ray Universe 2011 Symposium.
Conference LocationBerlin
Date27-30 June
PublisherESA
Tertiary TypeSessão Poster
History (UTC)2012-01-17 16:02:28 :: tereza@sid.inpe.br -> administrator :: 2011
2018-06-05 04:25:06 :: administrator -> tereza@sid.inpe.br :: 2011
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsX-ray emission
Magnetic Cataclysmic Variables
AbstractThe X-ray emission in magnetic cataclysmic variables is mainly due to an optically thin bremsstrahlung from the post-shock region. The observed flux of some systems shows variations along the orbital motion, which can be explained by phase-dependent absorption and/or occultation of the emitting regions. Two emitting regions can also play a role on these modulations. In this work, we explore these phase-dependent effects on the continuum emission of mCVs using CYCLOPS-X. This code calculates these effects self-consistently with the 3D geometry of the accretion column, limited by the lines of a dipolar magnetic field.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Phase-dependent effects on...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
agreement.html 02/12/2011 15:01 1.0 KiB 
4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP7W/3AT7M2S
zipped data URLhttp://urlib.net/zip/8JMKD3MGP7W/3AT7M2S
Languageen
Target FileSilva, Karleyne_TopicC-Congresso XrayUniverse 2011[1].pdf
User Groupadministrator
tereza@sid.inpe.br
Visibilityshown
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
LinkingTrabalho Vinculado à Tese/Dissertação
Mirror Repositorysid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Next Higher Units8JMKD3MGPCW/3ETR8EH
Citing Item Listsid.inpe.br/bibdigital/2013/10.01.00.07 3
sid.inpe.br/mtc-m21/2012/07.13.14.43.51 1
sid.inpe.br/mtc-m21/2012/07.13.14.51.06 1
URL (untrusted data)http://xmm.esac.esa.int/external/xmm_science/workshops/2011symposium/
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
Empty Fieldsarchivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi edition editor electronicmailaddress isbn issn label lineage mark nextedition notes numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress publisheraddress readergroup rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle sponsor subject type volume
7. Description control
e-Mail (login)tereza@sid.inpe.br
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