1. Identity statement | |
Reference Type | Journal Article |
Site | mtc-m21b.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 8JMKD3MGP3W34P/3NNBMEB |
Repository | sid.inpe.br/mtc-m21b/2017/04.17.18.33 |
Last Update | 2017:04.17.18.33.29 (UTC) administrator |
Metadata Repository | sid.inpe.br/mtc-m21b/2017/04.17.18.33.29 |
Metadata Last Update | 2018:06.04.02.27.23 (UTC) administrator |
DOI | 10.1093/mnras/stw3047 |
ISSN | 0035-8711 1365-2966 |
Citation Key | CáceresCarCoeLimRue:2017:ThXrEm |
Title | Thermal X-ray emission from massive, fast rotating, highly magnetized white dwarfs |
Year | 2017 |
Month | Mar. |
Access Date | 2024, Mar. 29 |
Type of Work | journal article |
Secondary Type | PRE PI |
Number of Files | 1 |
Size | 615 KiB |
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2. Context | |
Author | 1 Cáceres, D. L. 2 Carvalho, S. M. 3 Coelho, Jaziel Goulart 4 Lima, R. C. R. 5 Rueda, J. A. |
Group | 1 2 3 DIDAS-CGCEA-INPE-MCTIC-GOV-BR |
Affiliation | 1 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 Address | 1 2 3 jaziel.coelho@inpe.br |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 465 |
Number | 4 |
Pages | 4434-4440 |
Secondary Mark | A1_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 |
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3. Content and structure | |
Is the master or a copy? | is the master |
Content Stage | completed |
Transferable | 1 |
Content Type | External Contribution |
Version Type | publisher |
Keywords | acceleration of particles radiation mechanisms: thermal stars: magnetic field starspots white dwarfs |
Abstract | There 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. |
Area | CEA |
Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Thermal X-ray emission... |
doc Directory Content | access |
source Directory Content | there are no files |
agreement Directory Content | |
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4. Conditions of access and use | |
data URL | http://urlib.net/ibi/8JMKD3MGP3W34P/3NNBMEB |
zipped data URL | http://urlib.net/zip/8JMKD3MGP3W34P/3NNBMEB |
Language | en |
Target File | caceres_thermal.pdf |
User Group | self-uploading-INPE-MCTI-GOV-BR simone |
Visibility | shown |
Archiving Policy | allowpublisher allowfinaldraft |
Update Permission | not transferred |
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5. Allied materials | |
Linking | Trabalho não Vinculado à Tese/Dissertação |
Next Higher Units | 8JMKD3MGPCW/3ETR8EH |
Dissemination | WEBSCI; PORTALCAPES; MGA; COMPENDEX. |
Host Collection | sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 |
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6. Notes | |
Empty Fields | alternatejournal 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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7. Description control | |
e-Mail (login) | simone |
update | |
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