Published July 1981
| Version v1
Journal article
Radio-emitting supernovae as young plerions
Description
The radio emission observed in supernovae comes from young plerions formed immediately after the outbursts. As such a plerion expands, its radio power will decay approximately as R-1. Radio waves will be emitted only by supernovae of type II
Additional details
Publishing Information
- Journal Title
- Sov. Astron. Lett. (Engl. Transl.)
- Journal Volume
- 7
- Journal Issue
- 4
- Series
- Sov. Astron. Lett. (Engl. Transl.).
- Journal Page Range
- 263-264
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 13676770
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BRIGHTNESS; COSMIC RADIO SOURCES; POWER; RADIOWAVE RADIATION; SUPERNOVA REMNANTS; SUPERNOVAE
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; ERUPTIVE VARIABLE STARS; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; RADIATIONS; STARS; VARIABLE STARS