Paper:	Radio Emission from Supernovae
Volume:	342, 1604-2004: Supernovae as Cosmological Lighthouses
Page:	290
Authors:	Weiler, K.W.; Van Dyk, S.D.; Sramek, R.A.; Panagia, N.; Stockdale, C.J.; Montes M.J.
Abstract:	Study of radio supernovae over the past 25 years includes two dozen detected objects and more than 100 upper limits. From this work it is possible 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 detect clumpiness of the circumstellar material.

Astronomical Society of the Pacific
Conference Series

© Copyright 1988 - 2024 - Astronomical Society of the Pacific
No part of the material protected by this copyright may be reproduced or used in any form other than for personal use without written permission from the ASP.

Page generated in 0.073 seconds