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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/45LTBR8
Repositorysid.inpe.br/mtc-m21d/2021/10.25.18.55   (restricted access)
Last Update2021:10.25.19.01.49 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2021/10.25.18.55.10
Metadata Last Update2022:04.03.19.24.04 (UTC) administrator
DOI10.3847/1538-4365/ac141c
ISSN0067-0049
1538-4365
Label20211025
Citation KeyBelloniRSCCHLLMOPSSSZ:2021:BrDeMa
TitleBreaking the Degeneracy in Magnetic Cataclysmic Variable X-Ray Spectral Modeling Using X-Ray Light Curves
Year2021
MonthOCT
Access Date2024, May 01
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size3055 KiB
2. Context
Author 1 Belloni, Diogo Teixeira
 2 Rodrigues, Claudia Vilega
 3 Schreiber, Matthias R.
 4 Castro Avila, Manuel Antonio
 5 Costa, Joaquim Eduardo Rezende
 6 Hayashi, Takayuki
 7 Lima, Isabel de Jesus
 8 Luna, Gerardo J. M.
 9 Martins, Murilo
10 Oliveira, Alexandre S.
11 Parsons, Steven G.
12 Silva, Karleyne M. G.
13 Stecchini, Paulo Eduardo Freire
14 Stuchi, Teresa J.
15 Zorotovic, Monica
Resume Identifier 1
 2 8JMKD3MGP5W/3C9JGS5
 3
 4
 5 8JMKD3MGP5W/3C9JHF8
ORCID 1 0000-0003-1535-0866
 2 0000-0002-9459-043X
 3 0000-0003-3903-8009
 4 0000-0003-2162-8393
 5 0000-0002-0703-4735
 6
 7 0000-0001-6013-1772
 8 0000-0002-2647-4373
 9 0000-0003-3014-7989
10 0000-0001-6422-9486
11 0000-0002-2695-2654
12 0000-0003-1949-4621
13 0000-0002-2503-2434
14 0000-0003-0700-6205
15 0000-0002-4526-0469
Group 1 DIAST-CGCE-INPE-MCTI-GOV-BR
 2 DIAST-CGCE-INPE-MCTI-GOV-BR
 3
 4 DIAST-CGCE-INPE-MCTI-GOV-BR
 5 DICEP-CGCE-INPE-MCTI-GOV-BR
 6
 7 CGCE-CGCE-INPE-MCTI-GOV-BR
 8
 9
10
11
12
13 CGCE-CGCE-INPE-MCTI-GOV-BR
Affiliation 1 Instituto Nacional de Pesquisas Espaciais (INPE)
 2 Instituto Nacional de Pesquisas Espaciais (INPE)
 3 Universidad Técnica Federico Santa María
 4 Instituto Nacional de Pesquisas Espaciais (INPE)
 5 Instituto Nacional de Pesquisas Espaciais (INPE)
 6 NASA Goddard Space Flight Center
 7 Instituto Nacional de Pesquisas Espaciais (INPE)
 8 Universidad de Buenos Aires
 9 Universidade do Vale do Paraíba (UNIVAP)
10 Universidade do Vale do Paraíba (UNIVAP)
11 University of Sheffield
12 Gemini Observatory
13 Instituto Nacional de Pesquisas Espaciais (INPE)
14 Universidade Federal do Rio de Janeiro (UFRJ)
15 Universidad de Valparaíso
Author e-Mail Address 1 diogobellonizorzi@gmail.com
 2 claudia.vilega@gmail.com
 3
 4 castroavila_2004@hotmail.com
 5 jercosta@gmail.com
 6
 7 isabellima01@gmail.com
 8
 9
10
11
12
13 du.stecchini@gmail.com
JournalAstrophysical Journal Supplement Series
Volume256
Number2
Secondary MarkA1_ENGENHARIAS_III A1_ASTRONOMIA_/_FÍSICA A2_ENGENHARIAS_IV
History (UTC)2021-10-25 18:55:10 :: administrator -> simone ::
2021-10-25 19:01:50 :: simone -> administrator :: 2021
2021-10-25 19:01:50 :: administrator -> simone :: 2021
2021-10-25 19:02:01 :: simone -> administrator :: 2021
2022-04-03 19:24:04 :: administrator -> simone :: 2021
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractWe present an analysis of mock X-ray spectra and light curves of magnetic cataclysmic variables using an upgraded version of the 3D cyclops code. This 3D representation of the accretion flow allows us to properly model total and partial occultation of the postshock region by the white dwarf as well as the modulation of the X-ray light curves due to the phase-dependent extinction of the preshock region. We carried out detailed postshock region modeling in a four-dimensional parameter space by varying the white dwarf mass and magnetic field strength as well as the magnetosphere radius and the specific accretion rate. To calculate the postshock region temperature and density profiles, we assumed equipartition between ions and electrons; took into account the white dwarf gravitational potential, the finite size of the magnetosphere, and a dipole-like magnetic field geometry; and considered cooling by both bremsstrahlung and cyclotron radiative processes. By investigating the impact of the parameters on the resulting X-ray continuum spectra, we show that there is an inevitable degeneracy in the four-dimensional parameter space investigated here, which compromises X-ray continuum spectral fitting strategies and can lead to incorrect parameter estimates. However, the inclusion of X-ray light curves in different energy ranges can break this degeneracy, and it therefore remains, in principle, possible to use X-ray data to derive fundamental parameters of magnetic cataclysmic variables, which represents an essential step toward understanding their formation and evolution.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Breaking the Degeneracy...
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source Directory Contentthere are no files
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4. Conditions of access and use
Languageen
Target Filebelloni-Breaking.pdf
User Groupadministrator
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Reader Groupadministrator
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Visibilityshown
Archiving Policydenypublisher denyfinaldraft12
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/2022/04.03.17.52 2
sid.inpe.br/mtc-m21/2012/07.13.14.43.51 1
sid.inpe.br/mtc-m21/2012/07.13.14.51.06 1
DisseminationWEBSCI; PORTALCAPES.
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
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