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Supernovae at the Highest Angular Resolution

Published online by Cambridge University Press:  13 May 2016

Schuyler D. Van Dyk ,
K.W. Weiler ,
R.A. Sramek ,
N. Panagia ,
C.K. Lacey ,
M.J. Montes ,
J.M. Marcaide ,
W. H. G. Lewin ,
D.W. Fox  and
D. Pooley
...Show all authors
Schuyler D. Van Dyk
Affiliation:
IPAC/Caltech, 100-22, Pasadena, CA 91125 USA
K.W. Weiler
Affiliation:
NRL
R.A. Sramek
Affiliation:
NRAO
N. Panagia
Affiliation:
STScI
C.K. Lacey
Affiliation:
USC
M.J. Montes
Affiliation:
NRL
J.M. Marcaide
Affiliation:
Valencia
W. H. G. Lewin
Affiliation:
MIT
D.W. Fox
Affiliation:
MIT
D. Pooley
Affiliation:
MIT
A.V. Filippenko
Affiliation:
UC Berkeley
C.Y. Peng
Affiliation:
UAriz

Abstract

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The study of supernovae (SNe) and their environments in host galaxies at the highest possible angular resolution in a number of wavelength regimes is providing vital clues to the nature of their progenitor stars. We are observing SNe in the radio using the Very Large Array (VLA) and VLBI, in the X-rays with Chandra, and in the optical at the subarcsecond resolution of HST.

Type
Supernovae, Pulsars, and the Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 205: Galaxies and their Constituents at the Highest Angular Resolutions , 2001 , pp. 390 - 391
Copyright
Copyright © Astronomical Society of the Pacific 2001 

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