A time dependent approach to model X-ray and γ–ray light curves of Mrk 421 observed during the flare in February 2010

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dc.contributor.authorSingh, K. K.
dc.contributor.authorSahayanathan, S.
dc.contributor.authorSinha, A.
dc.contributor.authorBhatt, N.
dc.contributor.authorTickoo, A. K.
dc.contributor.authorYadav, K. K.
dc.contributor.authorRannot, R. C.
dc.contributor.authorChandra, P.
dc.contributor.authorVenugopal, K.
dc.contributor.authorMarandi, P.
dc.contributor.authorN. Kumar
dc.contributor.authorGoyal, H. C.
dc.contributor.authorGoyal, A.
dc.contributor.authorAgarwal, N. K.
dc.contributor.authorKothari, M.
dc.contributor.authorChanchalani, K.
dc.contributor.authorDhar, V. K.
dc.contributor.authorChouhan, N.
dc.contributor.authorBhat, C. K.
dc.contributor.authorKoul, M. K.
dc.contributor.authorKoul, R.
dc.date.accessioned2017-08-11T09:42:00Z
dc.date.available2017-08-11T09:42:00Z
dc.date.issued2017
dc.description.divisionApSDen
dc.format.extent5185 bytes
dc.format.mimetypetext/html
dc.identifier.sourceNew Astronomy, 2017. Vol. 54: pp. 24-29en
dc.identifier.urihttp://hdl.handle.net/123456789/14762
dc.language.isoenen
dc.subjectBL Lacertae objectsen
dc.subjectIndividualen
dc.subjectMrk 421-methodsen
dc.subjectData analysis-radiation mechanismsen
dc.subjectNon-thermalen
dc.titleA time dependent approach to model X-ray and γ–ray light curves of Mrk 421 observed during the flare in February 2010en
dc.typeArticleen

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