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Article: Correlation between the gamma-ray and the near-infrared emissions from gamma-ray-loud blazars in the low state

TitleCorrelation between the gamma-ray and the near-infrared emissions from gamma-ray-loud blazars in the low state
Authors
Zhang, XCheng, KSZhao, GHu, SM
Keywordsγ-rays: general: infared: observations
BL Lac object: general
Quasars: general
Issue Date2003
PublisherSpringer Verlag Dordrecht. The Journal's web site is located at http://springerlink.metapress.com/openurl.asp?genre=journal&issn=0004-640X
Citation
Astrophysics And Space Science, 2003, v. 286 n. 3-4, p. 323-331 How to Cite?
DOI: http://dx.doi.org/10.1023/A:1026331018507
AbstractWe have studied the correlations between the near-IR and the γ-ray bands using 29 observed γ-ray-loud blazars (16 BL Lac objects and 13 flat-spectrum radio quasars (FSRQs)) with near-IR and γ-ray spectral indices and fluxes. The results show that there are very strong correlations between near-IR mean spectral index αIR and γ-ray mean spectral index αγ and between near-IR and γ-ray fluxes. Which means that γ-ray radiation from the blazars should be mainly produced by the synchrotron self-Compton process. In addition, the γ-ray emission of BL Lac objects may be somewhat different from flat-spectrum radio quasars.
Persistent Identifierhttp://hdl.handle.net/10722/81030
ISSN
0004-640X
2021 Impact Factor: 1.909
2020 SCImago Journal Rankings: 0.398
ISI Accession Number ID
WOS:000185920900002
References
References in Scopus

 

DC FieldValueLanguage
dc.contributor.authorZhang, Xen_HK
dc.contributor.authorCheng, KSen_HK
dc.contributor.authorZhao, Gen_HK
dc.contributor.authorHu, SMen_HK
dc.date.accessioned2010-09-06T08:12:58Z-
dc.date.available2010-09-06T08:12:58Z-
dc.date.issued2003en_HK
dc.identifier.citationAstrophysics And Space Science, 2003, v. 286 n. 3-4, p. 323-331en_HK
dc.identifier.issn0004-640Xen_HK
dc.identifier.urihttp://hdl.handle.net/10722/81030-
dc.description.abstractWe have studied the correlations between the near-IR and the γ-ray bands using 29 observed γ-ray-loud blazars (16 BL Lac objects and 13 flat-spectrum radio quasars (FSRQs)) with near-IR and γ-ray spectral indices and fluxes. The results show that there are very strong correlations between near-IR mean spectral index αIR and γ-ray mean spectral index αγ and between near-IR and γ-ray fluxes. Which means that γ-ray radiation from the blazars should be mainly produced by the synchrotron self-Compton process. In addition, the γ-ray emission of BL Lac objects may be somewhat different from flat-spectrum radio quasars.en_HK
dc.languageengen_HK
dc.publisherSpringer Verlag Dordrecht. The Journal's web site is located at http://springerlink.metapress.com/openurl.asp?genre=journal&issn=0004-640Xen_HK
dc.relation.ispartofAstrophysics and Space Scienceen_HK
dc.subjectγ-rays: general: infared: observationsen_HK
dc.subjectBL Lac object: generalen_HK
dc.subjectQuasars: generalen_HK
dc.titleCorrelation between the gamma-ray and the near-infrared emissions from gamma-ray-loud blazars in the low stateen_HK
dc.typeArticleen_HK
dc.identifier.openurlhttp://library.hku.hk:4550/resserv?sid=HKU:IR&issn=0004-640X&volume=286&spage=323&epage=331&date=2003&atitle=Correlation+between+the+gamma-ray+and+the+near-infrared+emissions+from+gamma-ray-loud+blazars+in+the+low+stateen_HK
dc.identifier.emailCheng, KS: hrspksc@hkucc.hku.hken_HK
dc.identifier.authorityCheng, KS=rp00675en_HK
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1023/A:1026331018507en_HK
dc.identifier.scopuseid_2-s2.0-0345866968en_HK
dc.identifier.hkuros85375en_HK
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-0345866968&selection=ref&src=s&origin=recordpageen_HK
dc.identifier.volume286en_HK
dc.identifier.issue3-4en_HK
dc.identifier.spage323en_HK
dc.identifier.epage331en_HK
dc.identifier.isiWOS:000185920900002-
dc.publisher.placeNetherlandsen_HK
dc.identifier.scopusauthoridZhang, X=7410276524en_HK
dc.identifier.scopusauthoridCheng, KS=9745798500en_HK
dc.identifier.scopusauthoridZhao, G=7403296400en_HK
dc.identifier.scopusauthoridHu, SM=36818836400en_HK
dc.identifier.issnl0004-640X-

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