Close

1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/48LMC72
Repositorysid.inpe.br/mtc-m21d/2023/03.06.15.36   (restricted access)
Last Update2023:03.06.15.36.11 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2023/03.06.15.36.11
Metadata Last Update2024:01.02.17.16.41 (UTC) administrator
DOI10.3390/galaxies11010018
ISSN2075-4434
Citation KeySilvaLiCoStLiAr:2023:MeFiPh
TitleA method to fit phase diagrams of slow-rotation pulsars with accretion columns
Year2023
MonthFeb.
Access Date2024, May 12
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size1423 KiB
2. Context
Author1 Silva, Rodrigo R.
2 Lima, Rafael C. R. de
3 Coelho, Jaziel Goulart
4 Stecchini, Paulo Eduardo Freire
5 Liz, Caroline M. de
6 Araújo, José Carlos Neves de
Resume Identifier1
2
3
4
5
6 8JMKD3MGP5W/3C9JHGK
ORCID1
2 0000-0003-1718-3838
3 0000-0001-9386-1042
4
5
6 0000-0003-4418-4289
Group1 AST-CEA-DIPGR-INPE-MCTI-GOV-BR
2
3 DIAST-CGCE-INPE-MCTI-GOV-BR
4 DIAST-CGCE-INPE-MCTI-GOV-BR
5
6 DIAST-CGCE-INPE-MCTI-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Universidade do Estado de Santa Catarina (UDESC)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 Universidade do Estado de Santa Catarina (UDESC)
6 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1
2 rafael.lima@udesc.br
3
4 du.stecchini@gmail.com
5
6 jcndearaujo@gmail.com
JournalGalaxies
Volume11
Number1
Pagese18
History (UTC)2023-03-06 15:36:41 :: simone -> administrator :: 2023
2024-01-02 17:16:41 :: administrator -> simone :: 2023
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywords1A 0535+262
accretion column
pulse profile
AbstractWe demonstrate a method to simulate a pulse profile of the emission of accretion columns in a neutron star. Given a set of parameters that characterize the star, e.g., mass and radius, and the positions and shapes of the accretion columns, the pulse profile can be calculated and compared with real data. Some characteristics of phase diagrams are shown considering an accretion column in the form of a cone trunk and also in the form of a cylinder. Furthermore, in our first approach we develop a combination between a genetic algorithm and a Bayesian sampling algorithm to constrain some variables. Finally, as an example, we apply the method to observed data of source 1A 0535+262.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > AST > A method to...
Arrangement 2urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > A method to...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
agreement.html 06/03/2023 12:36 1.0 KiB 
4. Conditions of access and use
Languageen
Target Filegalaxies-11-00018.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3F2NE4L
8JMKD3MGPCW/46KTFK8
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.51.44 1
sid.inpe.br/bibdigital/2013/10.12.16.06 1
sid.inpe.br/bibdigital/2022/04.03.17.52 1
DisseminationWEBSCI; PORTALCAPES; SCOPUS.
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
Empty Fieldsalternatejournal archivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark mirrorrepository nextedition notes parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey secondarymark session shorttitle sponsor subject tertiarymark tertiarytype url
7. Description control
e-Mail (login)simone
update 


Close