Astronomy and Astrophysics – Astrophysics
Scientific paper
May 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..565..237w&link_type=abstract
YOUNG SUPERNOVA REMNANTS: Eleventh Astrophysics Conference. AIP Conference Proceedings, Volume 565, pp. 237-246 (2001).
Astronomy and Astrophysics
Astrophysics
1
Supernovae, Supernova Remnants, Pulsars
Scientific paper
Study of radio supernovae (RSNe), the earliest stages of supernova remnant (SNR) formation, over the past 20 years includes two dozen detected objects and more than 100 upper limits. From this work we are able to identify classes of radio properties, demonstrate conformance to and deviations from existing models, estimate the density and structure of the circumstellar material and, by inference, the evolution of the presupernova stellar wind, and reveal the last stages of stellar evolution before explosion. It is also possible to detect ionized hydrogen along the line of sight, to demonstrate binary properties of the stellar system, and to show clumpiness of the circumstellar material. More speculatively, it may be possible to provide distance estimates to RSNe. .
Lacey Christina K.
Montes Marcos J.
Panagia Nino
Sramek Richard A.
Van Dyk Schuyler D.
No associations
LandOfFree
Radio emission from SNe and young SNRs 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 Radio emission from SNe and young SNRs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radio emission from SNe and young SNRs will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1279723