Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apj...466..808z&link_type=abstract
Astrophysical Journal v.466, p.808
Astronomy and Astrophysics
Astronomy
3
Ism: Bubbles, Ism: Structure, Stars: Mass Loss, Ism: Supernova Remnants
Scientific paper
The evolution and nonthermal radio emission of Type Ib and II supernova remnants can be strikingly affected by the circumstellar winds blown out from their massive progenitor stars. For the supernova remnants evolving in the freely expanding and shocked wind regions which are considered to have toroidal magnetic structure, besides the flow, the internal magnetic field has a self-similar solution. In this case, at different aspect angles, the synchrotron emission of the remnant demonstrates a variety of shapes, including "center-brightened," "double-lobed," "bilateral-brightened," and the normal "shellshaped," which can be used to interpret some unusual morphologies of young supernova remnants.
Chen Yang
Wang Zhenru
Zhang Qing-Chun
No associations
LandOfFree
A Self-similar Solution for the Magnetic Field Distribution of Supernova Remnants Evolving in Stellar Wind Bubbles and Their Corresponding Radio Morphologies does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with A Self-similar Solution for the Magnetic Field Distribution of Supernova Remnants Evolving in Stellar Wind Bubbles and Their Corresponding Radio Morphologies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Self-similar Solution for the Magnetic Field Distribution of Supernova Remnants Evolving in Stellar Wind Bubbles and Their Corresponding Radio Morphologies will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1448381