Article contents
Supernovae at the Highest Angular Resolution
Published online by Cambridge University Press: 13 May 2016
Abstract
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
- Copyright
- Copyright © Astronomical Society of the Pacific 2001
References
- 3
- Cited by