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Article: The complex wind torus and jets of PSR B1706-44

TitleThe complex wind torus and jets of PSR B1706-44
Authors
Romani, RWNg, CYDodson, RBrisken, W
Issue Date2005
PublisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/0004-637X
Citation
Astrophysical Journal, 2005, v. 631 n. 1 I, p. 480-487 How to Cite?
DOI: http://dx.doi.org/10.1086/432527
AbstractWe report on Chandra ACIS imaging of the pulsar wind nebula (PWN) of the young Vela-like PSR B1706-44, which shows the now common pattern of an equatorial wind and polar jets. The structure is particularly rich, showing a relativistically boosted termination shock, jets with strong confinement, a surrounding radio/X-ray PWN, and evidence for a quasistatic "bubble nebula." The structures trace the pulsar spin geometry and illuminate its possible relation to SNR G343.1-2.3. We also obtain improved estimates of the pulsar flux and nebular spectrum, constraining the system age and energetics. © 2005. The American Astronomical Society. All rights reserved.
Persistent Identifierhttp://hdl.handle.net/10722/180482
ISSN
0004-637X
2023 Impact Factor: 4.8
2023 SCImago Journal Rankings: 1.905
ISI Accession Number ID
WOS:000231959100036
References
References in Scopus

 

DC FieldValueLanguage
dc.contributor.authorRomani, RWen_US
dc.contributor.authorNg, CYen_US
dc.contributor.authorDodson, Ren_US
dc.contributor.authorBrisken, Wen_US
dc.date.accessioned2013-01-28T01:38:44Z-
dc.date.available2013-01-28T01:38:44Z-
dc.date.issued2005en_US
dc.identifier.citationAstrophysical Journal, 2005, v. 631 n. 1 I, p. 480-487en_US
dc.identifier.issn0004-637Xen_US
dc.identifier.urihttp://hdl.handle.net/10722/180482-
dc.description.abstractWe report on Chandra ACIS imaging of the pulsar wind nebula (PWN) of the young Vela-like PSR B1706-44, which shows the now common pattern of an equatorial wind and polar jets. The structure is particularly rich, showing a relativistically boosted termination shock, jets with strong confinement, a surrounding radio/X-ray PWN, and evidence for a quasistatic "bubble nebula." The structures trace the pulsar spin geometry and illuminate its possible relation to SNR G343.1-2.3. We also obtain improved estimates of the pulsar flux and nebular spectrum, constraining the system age and energetics. © 2005. The American Astronomical Society. All rights reserved.en_US
dc.languageengen_US
dc.publisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/0004-637Xen_US
dc.relation.ispartofAstrophysical Journalen_US
dc.titleThe complex wind torus and jets of PSR B1706-44en_US
dc.typeArticleen_US
dc.identifier.emailNg, CY: stephen_ng@hku.hken_US
dc.identifier.authorityNg, CY=rp01706en_US
dc.description.naturelink_to_OA_fulltexten_US
dc.identifier.doi10.1086/432527en_US
dc.identifier.scopuseid_2-s2.0-27744438479en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-27744438479&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume631en_US
dc.identifier.issue1 Ien_US
dc.identifier.spage480en_US
dc.identifier.epage487en_US
dc.identifier.isiWOS:000231959100036-
dc.publisher.placeUnited Kingdomen_US
dc.identifier.scopusauthoridRomani, RW=35248859100en_US
dc.identifier.scopusauthoridNg, CY=24830903500en_US
dc.identifier.scopusauthoridDodson, R=7102372205en_US
dc.identifier.scopusauthoridBrisken, W=6602418286en_US
dc.customcontrol.immutablejt 130807-
dc.identifier.issnl0004-637X-

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