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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34P/3NNBMEB
Repositorysid.inpe.br/mtc-m21b/2017/04.17.18.33
Last Update2017:04.17.18.33.29 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21b/2017/04.17.18.33.29
Metadata Last Update2018:06.04.02.27.23 (UTC) administrator
DOI10.1093/mnras/stw3047
ISSN0035-8711
1365-2966
Citation KeyCáceresCarCoeLimRue:2017:ThXrEm
TitleThermal X-ray emission from massive, fast rotating, highly magnetized white dwarfs
Year2017
MonthMar.
Access Date2024, Mar. 29
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size615 KiB
2. Context
Author1 Cáceres, D. L.
2 Carvalho, S. M.
3 Coelho, Jaziel Goulart
4 Lima, R. C. R.
5 Rueda, J. A.
Group1
2
3 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Sapienza Università di Roma
2 Universidade Federal do Tocantins (UFTO)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 ICRANet
5 Sapienza Università di Roma
Author e-Mail Address1
2
3 jaziel.coelho@inpe.br
JournalMonthly Notices of the Royal Astronomical Society
Volume465
Number4
Pages4434-4440
Secondary MarkA1_QUÍMICA A1_INTERDISCIPLINAR A1_GEOCIÊNCIAS A1_ENGENHARIAS_III A2_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA A2_ASTRONOMIA_/_FÍSICA B2_ENSINO B5_ENGENHARIAS_IV
History (UTC)2017-04-17 18:33:29 :: simone -> administrator ::
2018-06-04 02:27:23 :: administrator -> simone :: 2017
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsacceleration of particles
radiation mechanisms: thermal
stars: magnetic field
starspots
white dwarfs
AbstractThere is solid observational evidence on the existence of massive, M similar to 1M(circle dot), highly magnetized white dwarfs (WDs) with surface magnetic fields up to B similar to 10(9) G. We show that, if in addition to these features, the star is fast rotating, it can become a rotation-powered pulsar-like WD and emit detectable high-energy radiation. We infer the values of the structure parameters (mass, radius, moment of inertia), magnetic field, rotation period and spin-down rates of a WD pulsar death-line. We show that WDs above the death-line emit blackbody radiation in the soft X-ray band via the magnetic polar cap heating by back flowing pair-created particle bombardment and discuss as an example the X-ray emission of soft gamma-repeaters and anomalous X-ray pulsars within the WD model.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Thermal X-ray emission...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
agreement.html 17/04/2017 15:33 1.0 KiB 
4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34P/3NNBMEB
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34P/3NNBMEB
Languageen
Target Filecaceres_thermal.pdf
User Groupself-uploading-INPE-MCTI-GOV-BR
simone
Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
Update Permissionnot transferred
5. Allied materials
LinkingTrabalho não Vinculado à Tese/Dissertação
Next Higher Units8JMKD3MGPCW/3ETR8EH
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionsid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup readpermission resumeid rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarytype url
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