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Article: On the radio emission following the August 27 giant flare of SGR 1900+14

TitleOn the radio emission following the August 27 giant flare of SGR 1900+14
Authors
Ertan, ÜCheng, KS
KeywordsAccretion: accretion disks
ISM: jets and outflows
Pulsars: individual: SGR 1900+14
Stars: neutron
X-rays: bursts
Issue Date2004
PublisherElsevier BV. The Journal's web site is located at http://www.elsevier.com/locate/newast
Citation
New Astronomy, 2004, v. 9 n. 7, p. 503-507 How to Cite?
DOI: http://dx.doi.org/10.1016/j.newast.2004.02.005
AbstractBy comparing our analytical estimates with the results of the model fits to the radio data of the SGR 1900+14, we show that the radio afterglow of the August 27 giant flare of this source can be accounted for by the outflow of inner disk matter by the flare pressure. Our results are consistent with the observed flare energy and its estimated fraction imparted to the inner disk. © 2004 Elsevier B.V. All rights reserved.
Persistent Identifierhttp://hdl.handle.net/10722/80740
ISSN
1384-1076
2023 Impact Factor: 1.9
2023 SCImago Journal Rankings: 0.476
ISI Accession Number ID
WOS:000224734500001
References
References in Scopus

 

DC FieldValueLanguage
dc.contributor.authorErtan, Üen_HK
dc.contributor.authorCheng, KSen_HK
dc.date.accessioned2010-09-06T08:09:45Z-
dc.date.available2010-09-06T08:09:45Z-
dc.date.issued2004en_HK
dc.identifier.citationNew Astronomy, 2004, v. 9 n. 7, p. 503-507en_HK
dc.identifier.issn1384-1076en_HK
dc.identifier.urihttp://hdl.handle.net/10722/80740-
dc.description.abstractBy comparing our analytical estimates with the results of the model fits to the radio data of the SGR 1900+14, we show that the radio afterglow of the August 27 giant flare of this source can be accounted for by the outflow of inner disk matter by the flare pressure. Our results are consistent with the observed flare energy and its estimated fraction imparted to the inner disk. © 2004 Elsevier B.V. All rights reserved.en_HK
dc.languageengen_HK
dc.publisherElsevier BV. The Journal's web site is located at http://www.elsevier.com/locate/newasten_HK
dc.relation.ispartofNew Astronomyen_HK
dc.rightsNew Astronomy. Copyright © Elsevier BV.en_HK
dc.subjectAccretion: accretion disksen_HK
dc.subjectISM: jets and outflowsen_HK
dc.subjectPulsars: individual: SGR 1900+14en_HK
dc.subjectStars: neutronen_HK
dc.subjectX-rays: burstsen_HK
dc.titleOn the radio emission following the August 27 giant flare of SGR 1900+14en_HK
dc.typeArticleen_HK
dc.identifier.openurlhttp://library.hku.hk:4550/resserv?sid=HKU:IR&issn=1384-1076&volume=9&spage=503&epage=507&date=2004&atitle=On+the+radio+emission+following+the+August+27+giant+flare+of+SGR+1900+14en_HK
dc.identifier.emailCheng, KS: hrspksc@hkucc.hku.hken_HK
dc.identifier.authorityCheng, KS=rp00675en_HK
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1016/j.newast.2004.02.005en_HK
dc.identifier.scopuseid_2-s2.0-2542491578en_HK
dc.identifier.hkuros91988en_HK
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-2542491578&selection=ref&src=s&origin=recordpageen_HK
dc.identifier.volume9en_HK
dc.identifier.issue7en_HK
dc.identifier.spage503en_HK
dc.identifier.epage507en_HK
dc.identifier.isiWOS:000224734500001-
dc.publisher.placeNetherlandsen_HK
dc.identifier.scopusauthoridErtan, Ü=36486249800en_HK
dc.identifier.scopusauthoridCheng, KS=9745798500en_HK
dc.identifier.issnl1384-1076-

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