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Article: Gamma-ray activity in the crab nebula: The exceptional flare of 2011 April

TitleGamma-ray activity in the crab nebula: The exceptional flare of 2011 April
Authors
Buehler, RScargle, JDBlandford, RDBaldini, LBaring, MGBelfiore, ACharles, EChiang, JD'ammando, FDermer, CDFunk, SGrove, JEHarding, AKHays, EKerr, MMassaro, FMazziotta, MNRomani, RWSaz Parkinson, PMTennant, AFWeisskopf, MC
KeywordsGamma Rays: Stars
Ism: Supernova Remnants
Magnetic Reconnection
Magnetohydrodynamics (Mhd)
Pulsars: Individual (Crab)
Radiation Mechanisms: Non-Thermal
Issue Date2012
PublisherInstitute of Physics Publishing, Inc. The Journal's web site is located at http://iopscience.iop.org/0004-637X/
Citation
Astrophysical Journal, 2012, v. 749 n. 1 How to Cite?
DOI: http://dx.doi.org/10.1088/0004-637X/749/1/26
AbstractThe Large Area Telescope on board the Fermi satellite observed a gamma-ray flare in the Crab Nebula lasting for approximately nine days in April of 2011. The source, which at optical wavelengths has a size of 11 lt-yr across, doubled its gamma-ray flux within eight hours. The peak photon flux was (186 6) × 10 -7cm -2s -1 above 100MeV, which corresponds to a 30-fold increase compared to the average value. During the flare, a new component emerged in the spectral energy distribution, which peaked at an energy of (375 26)MeV at flare maximum. The observations imply that the emission region was likely relativistically beamed toward us and that variations in its motion are responsible for the observed spectral variability. © 2012. The American Astronomical Society. All rights reserved.
Persistent Identifierhttp://hdl.handle.net/10722/188417
ISSN
0004-637X
2023 Impact Factor: 4.8
2023 SCImago Journal Rankings: 1.905
ISI Accession Number ID
WOS:000302175500026
References
References in Scopus

 

DC FieldValueLanguage
dc.contributor.authorBuehler, Ren_US
dc.contributor.authorScargle, JDen_US
dc.contributor.authorBlandford, RDen_US
dc.contributor.authorBaldini, Len_US
dc.contributor.authorBaring, MGen_US
dc.contributor.authorBelfiore, Aen_US
dc.contributor.authorCharles, Een_US
dc.contributor.authorChiang, Jen_US
dc.contributor.authorD'ammando, Fen_US
dc.contributor.authorDermer, CDen_US
dc.contributor.authorFunk, Sen_US
dc.contributor.authorGrove, JEen_US
dc.contributor.authorHarding, AKen_US
dc.contributor.authorHays, Een_US
dc.contributor.authorKerr, Men_US
dc.contributor.authorMassaro, Fen_US
dc.contributor.authorMazziotta, MNen_US
dc.contributor.authorRomani, RWen_US
dc.contributor.authorSaz Parkinson, PMen_US
dc.contributor.authorTennant, AFen_US
dc.contributor.authorWeisskopf, MCen_US
dc.date.accessioned2013-09-03T04:05:41Z-
dc.date.available2013-09-03T04:05:41Z-
dc.date.issued2012en_US
dc.identifier.citationAstrophysical Journal, 2012, v. 749 n. 1en_US
dc.identifier.issn0004-637Xen_US
dc.identifier.urihttp://hdl.handle.net/10722/188417-
dc.description.abstractThe Large Area Telescope on board the Fermi satellite observed a gamma-ray flare in the Crab Nebula lasting for approximately nine days in April of 2011. The source, which at optical wavelengths has a size of 11 lt-yr across, doubled its gamma-ray flux within eight hours. The peak photon flux was (186 6) × 10 -7cm -2s -1 above 100MeV, which corresponds to a 30-fold increase compared to the average value. During the flare, a new component emerged in the spectral energy distribution, which peaked at an energy of (375 26)MeV at flare maximum. The observations imply that the emission region was likely relativistically beamed toward us and that variations in its motion are responsible for the observed spectral variability. © 2012. The American Astronomical Society. All rights reserved.en_US
dc.languageengen_US
dc.publisherInstitute of Physics Publishing, Inc. The Journal's web site is located at http://iopscience.iop.org/0004-637X/en_US
dc.relation.ispartofAstrophysical Journalen_US
dc.subjectGamma Rays: Starsen_US
dc.subjectIsm: Supernova Remnantsen_US
dc.subjectMagnetic Reconnectionen_US
dc.subjectMagnetohydrodynamics (Mhd)en_US
dc.subjectPulsars: Individual (Crab)en_US
dc.subjectRadiation Mechanisms: Non-Thermalen_US
dc.titleGamma-ray activity in the crab nebula: The exceptional flare of 2011 Aprilen_US
dc.typeArticleen_US
dc.identifier.emailSaz Parkinson, PM: pablosp@hku.hken_US
dc.identifier.authoritySaz Parkinson, PM=rp01803en_US
dc.description.naturelink_to_subscribed_fulltexten_US
dc.identifier.doi10.1088/0004-637X/749/1/26en_US
dc.identifier.scopuseid_2-s2.0-84858964121en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-84858964121&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume749en_US
dc.identifier.issue1en_US
dc.identifier.isiWOS:000302175500026-
dc.publisher.placeUnited Statesen_US
dc.identifier.scopusauthoridBuehler, R=55138489700en_US
dc.identifier.scopusauthoridScargle, JD=6603849454en_US
dc.identifier.scopusauthoridBlandford, RD=35228413700en_US
dc.identifier.scopusauthoridBaldini, L=35748339500en_US
dc.identifier.scopusauthoridBaring, MG=7003670883en_US
dc.identifier.scopusauthoridBelfiore, A=26535417200en_US
dc.identifier.scopusauthoridCharles, E=7103332011en_US
dc.identifier.scopusauthoridChiang, J=24586575400en_US
dc.identifier.scopusauthoridD'Ammando, F=6505606078en_US
dc.identifier.scopusauthoridDermer, CD=7005781264en_US
dc.identifier.scopusauthoridFunk, S=8238179000en_US
dc.identifier.scopusauthoridGrove, JE=7103266596en_US
dc.identifier.scopusauthoridHarding, AK=55138522200en_US
dc.identifier.scopusauthoridHays, E=35229539600en_US
dc.identifier.scopusauthoridKerr, M=35229880000en_US
dc.identifier.scopusauthoridMassaro, F=16305108300en_US
dc.identifier.scopusauthoridMazziotta, MN=55139003400en_US
dc.identifier.scopusauthoridRomani, RW=55140366700en_US
dc.identifier.scopusauthoridSaz Parkinson, PM=8948464400en_US
dc.identifier.scopusauthoridTennant, AF=7006183262en_US
dc.identifier.scopusauthoridWeisskopf, MC=7005528199en_US
dc.identifier.issnl0004-637X-

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