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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34P/3PE7E6P
Repositorysid.inpe.br/mtc-m21b/2017/08.11.16.02   (restricted access)
Last Update2017:08.11.16.02.33 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21b/2017/08.11.16.02.33
Metadata Last Update2018:06.04.02.27.42 (UTC) administrator
DOI10.3847/2041-8213/aa7942
ISSN2041-8205
2041-8213
Citation KeyStecchiniCasJabD’ABra:2017:TaSwIN
TitleTandem swift and INTEGRAL data to revisit the orbital and superorbital periods of 1E1740.7-2942
Year2017
Access Date2024, May 18
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size705 KiB
2. Context
Author1 Stecchini, Paulo Eduardo Freire
2 Castro, Manuel
3 Jablonski, Francisco José
4 D’Amico, Flávio
5 Braga, João
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JH4Q
4
5 8JMKD3MGP5W/3C9JHEK
Group1 AST-CEA-SESPG-INPE-MCTIC-GOV-BR
2 AST-CEA-SESPG-INPE-MCTIC-GOV-BR
3 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
4 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
5 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 paulo.stecchini@inpe.br
2
3 f.jablonski@inpe.br
4 flavio.damico@inpe.br
5 joao.braga@inpe.br
JournalAstrophysical Journal Letters
Volume843
Number1
Secondary MarkA1_GEOCIÊNCIAS A1_ENGENHARIAS_III A2_ENGENHARIAS_IV A2_ASTRONOMIA_/_FÍSICA
History (UTC)2017-08-11 16:02:33 :: simone -> administrator ::
2017-08-11 16:02:34 :: administrator -> simone :: 2017
2017-08-11 16:03:40 :: simone -> administrator :: 2017
2018-06-04 02:27:42 :: administrator -> simone :: 2017
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsJuly
AbstractThe black hole candidate 1E 1740.7-2942 is one of the strongest hard X-ray sources in the Galactic Center region. No counterparts in longer wavelengths have been identified for this object yet. The presence of characteristic timing signatures in the flux history of X-ray sources has been shown to be an important diagnostic tool for the properties of these systems. Using simultaneous data from NASA's Swift and ESA's INTEGRAL missions, we have found two periodic signatures at 12.61 +/- 0.06 days and 171.1 +/- 3.0 days in long-term hard X-ray light curves of 1E 1740.7-2942. We interpret those as the orbital and superorbital periods of the object, respectively. The reported orbital period is in good agreement with previous studies of 1E 1740.7-2942 using NASA's RXTE data. We present here the first firm evidence of a superorbital period for 1E 1740.7-2942, which has important implications for the nature of the binary system.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Tandem swift and...
Arrangement 2urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > AST > Tandem swift and...
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4. Conditions of access and use
Languageen
Target Filestecchini_tandem.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policydenypublisher denyfinaldraft
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Linking8JMKD3MGP3W34P/3NFLPDL
Mirror Repositorysid.inpe.br/mtc-m21b/2013/09.26.14.25.22
Next Higher Units8JMKD3MGPCW/3ETR8EH
8JMKD3MGPCW/3F2NE4L
Citing Item List
DisseminationWEBSCI; PORTALCAPES; SCOPUS.
Host Collectionsid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notes
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