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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZGivnK2Y/QeqL5
Repositorysid.inpe.br/mtc-m17@80/2007/05.23.17.27   (restricted access)
Last Update2007:05.23.17.27.35 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m17@80/2007/05.23.17.27.37
Metadata Last Update2018:06.05.03.34.09 (UTC) administrator
Secondary KeyINPE--PRE/
ISSN0004-6256
Citation KeyRodriguesHickCerqTarg:2007:OpPoHH
TitleOptical polarimetry of HH 135/HH 136
Year2007
Monthmay
Access Date2024, Apr. 28
Secondary TypePRE PI
Number of Files1
Size1605 KiB
2. Context
Author1 Rodrigues, Cláudia Vilega
2 Hickel, G. R.
3 Cerqueira, A. H.
4 Targon, Cristiane Godoy
Group1 DAS-INPE-MCT-BR
2
3
4 DAS-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Universidade do Vale do Paraíba (UNIVAP)
3 Universidade Estadual de Santa Cruz
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 claudiavr@das.inpe.br
JournalAstronomical Journal
Volume133
Number5
Pages2334-2342
History (UTC)2007-06-13 11:05:13 :: simone -> administrator ::
2010-05-11 02:08:21 :: administrator -> simone ::
2010-05-18 13:14:00 :: simone -> administrator ::
2012-10-23 23:52:45 :: administrator -> simone :: 2007
2013-02-20 15:19:57 :: simone -> administrator :: 2007
2018-06-05 03:34:09 :: administrator -> marciana :: 2007
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsISM: Herbig-Haro objects
ISM: individual (HH 135
HH 136)
ISM: magnetic fields
ASTROPHYSICS
AbstractWe present optical linear polarimetry in the line of sight to HH 135/HH 136. The polarimetry of the field stars reveals two populations: one corresponds to a foreground interstellar component; the other originates in the interstellar medium in the vicinity of the Herbig-Haro pair and, therefore, can be used to study the magnetic field in the star-forming region. Its direction is aligned with the jet of HH 135/HH 136, which could be an indication that the interstellar magnetic field is important in the outflow collimation. The interstellar magnetic field magnitude was estimated to be of order 90 uG. According to recent numerical simulations, an interstellar magnetic field of such strength can be important in the definition of the outflow direction. There is also evidence that the associated dark cloud has an elongation parallel to the magnetic field. Our image polarimetry of the extended emission associated with HH 135/HH 136 shows a centrosymmetric pattern pointing to knot E of HH 136. Previous near-infrared polarimetry traces a different illumination center, namely, IRAS 11101-5829, the probable exciting source of the system. This discrepancy can be explained if the young stellar object emission is completely blocked in optical wavelengths and the dominant optical source in the region is knot E, whose nature is uncertain. A discussion of the spectral energy distributions of HH 136-E and IRAS 11101-5829 is presented.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Optical polarimetry of...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target FileOptical_rodrigues.pdf
User Groupadministrator
simone
Visibilityshown
Archiving Policydenypublisher denyfinaldraft
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
DisseminationWEBSCI; PORTALCAPES.
Host Collectionlcp.inpe.br/ignes/2004/02.12.18.39
cptec.inpe.br/walmeida/2003/04.25.17.12
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel documentstage doi e-mailaddress format isbn label lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype
7. Description control
e-Mail (login)marciana
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