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

Singh, K. K.Sahayanathan, S.Sinha, A.Bhatt, N.Tickoo, A. K.Yadav, K. K.Rannot, R. C.Chandra, P.Venugopal, K.Marandi, P.N. KumarGoyal, H. C.Goyal, A.Agarwal, N. K.Kothari, M.Chanchalani, K.Dhar, V. K.Chouhan, N.Bhat, C. K.Koul, M. K.Koul, R.2017-08-112017-08-112017New Astronomy, 2017. Vol. 54: pp. 24-29http://hdl.handle.net/123456789/147625185 bytestext/htmlenBL Lacertae objectsIndividualMrk 421-methodsData analysis-radiation mechanismsNon-thermalA time dependent approach to model X-ray and γ–ray light curves of Mrk 421 observed during the flare in February 2010Article