Time Dependent Model of Young Pulsar Wind Nebulae

A.Chatterjee1*, L. Saha2 and P. Majumdar1
1Saha Institute of Nuclear Physics, 1/AF Bidhannagar, Kolkata, India
2Tata Institute of Fundamental Research, Colaba, Mumbai, India

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Abstract

A time dependent leptonic model is developed in order to explain the broadband non-thermal radiation from pulsar wind nebulae.

Fig. 1


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