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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/45LTDNB
Repositorysid.inpe.br/mtc-m21d/2021/10.25.19.18
Last Update2021:10.25.19.18.17 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2021/10.25.19.18.17
Metadata Last Update2022:04.03.19.24.04 (UTC) administrator
DOI10.3847/1538-4357/ac1d41
ISSN0004-637X
1538-4357
Citation KeyCoelhoAraúLadiNune:2021:CaCrVe
TitleObservational Constraints on the Pulsar Wind Model: The Cases of Crab and Vela
Year2021
MonthOct.
Access Date2024, May 07
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size389 KiB
2. Context
Author1 Coelho, Jaziel G.
2 Araújo, José Carlos Neves de
3 Ladislau, Samantha Monaliza
4 Nunes, Rafael da Costa
Resume Identifier1
2 8JMKD3MGP5W/3C9JHGK
ORCID1 0000-0001-9386-1042
Group1
2 DIAST-CGCE-INPE-MCTI-GOV-BR
3 DIAST-CGCE-INPE-MCTI-GOV-BR
4 DIAST-CGCE-INPE-MCTI-GOV-BR
Affiliation1 Universidade Tecnológica Federal do Paraná (UTFPR)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 jazielcoelho@utfpr.edu.br
2 jcndearaujo@gmail.com
3 smladislau@gmail.com
4 rafadcnunes@gmail.com
JournalAstrophysical Journal
Volume920
Number1
Pagese57
Secondary MarkA1_QUÍMICA A1_INTERDISCIPLINAR A1_GEOCIÊNCIAS A1_ENGENHARIAS_III A1_ASTRONOMIA_/_FÍSICA A2_ENGENHARIAS_IV B2_ENSINO
History (UTC)2021-10-25 19:18:17 :: simone -> administrator ::
2021-10-25 19:18:18 :: administrator -> simone :: 2021
2021-10-25 19:18:38 :: 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
AbstractAs is well known, pulsars are extremely stable rotators. However, although slowly, they spindown thanks to brake mechanisms, which are in fact still a subject of intense investigation in the literature. Since pulsars are usually modeled as highly magnetized neutron stars that emit beams of electromagnetic radiation out of their magnetic poles, it is reasonable to consider that the spindown has to do with a magnetic brake. Although an interesting and simple idea, a pure magnetic brake is not able to adequately account for the spindown rate. Thus, many alternative spindown mechanisms appear in the literature, among them the pulsar wind model, where the wind of particles coming from the pulsar itself can carry part of its rotational kinetic energy. Such a spindown mechanism depends critically on three parameters, namely, the dipole magnetic field (B), the angle between the magnetic and rotation axes (phi), and the density of primary particles (zeta) of the pulsar's magnetosphere. Differently from a series of articles in this subject, we consider for the first time in the literature a statistical modeling that includes a combination of a magnetic dipole and wind brakes. As a result, we are able to constrain the above referred parameters in particular for Crab and Vela pulsars.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Observational Constraints on...
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source Directory Contentthere are no files
agreement Directory Content
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34T/45LTDNB
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34T/45LTDNB
Languageen
Target Filecoelho_observational.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
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-m21/2012/07.13.14.51.44 1
DisseminationWEBSCI; PORTALCAPES; COMPENDEX; SCOPUS.
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
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