Vela X is a pulsar wind nebula (PWN) associated with the active pulsar B0833-45 and contained within the Vela supernova remnant (SNR). A collimated X-ray filament (“cocoon”) extends south-southwest from the pulsar to the center of Vela X. VLA observations uncovered radio emission coincident with the eastern edge of the cocoon and H.E.S.S. has detected TeV γ-ray emission from this region as well...

The activity of sericulture is declining due the reduction of mulberry production area in sericulture practicing countries lead to adverse effects on silkworm rearing and cocoon production. Screening for nutrigenetic traits in silkworm, Bombyx mori L. (Lepidoptera: Bombycidae) is an essential prerequisite for better understanding and development of nutritionally efficient breeds/hybrids, which ...

ROSAT observations of the Vela pulsar and its surroundings revealed a collimated X-ray feature almost 45 in length (Markwardt & Ögelman 1995), interpreted as the signature “cocoon” of a one-sided jet from the Vela pulsar. We report on a new ASCA observation of the Vela pulsar jet at its head, the point where the jet is believed to interact with the supernova remnant. The head is clearly detecte...

ABSTRACT We have simulated the evolution of non-thermal cosmic ray electrons (CREs) in 3D relativistic magneto hydrodynamic (MHD) jets evolved up to a height 9 kpc. The CREs been space and energy concurrently with jet fluid, duly accounting for radiative losses acceleration at shocks. show that stable MHD instabilities expected trends regular flow spine hotspot followed by settling backflow. Ho...