Skip to main content
OSTI.GOVU.S. Department of Energy Office of Scientific and Technical Information
U.S. Department of Energy
Office of Scientific and Technical Information
 

Radio-emitting supernovae as young plerions

Journal Article · · Sov. Astron. Lett. (Engl. Transl.); (United States)
OSTI ID:5792134
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/sup -1/. Radio waves will be emitted only by supernovae of type II.
Research Organization:
Inst. for Space Research, USSR Academy of Sciences, Moscow
OSTI ID:
5792134
Journal Information:
Sov. Astron. Lett. (Engl. Transl.); (United States), Journal Name: Sov. Astron. Lett. (Engl. Transl.); (United States) Vol. 7:4; ISSN SALED
Country of Publication:
United States
Language:
English

Similar Records

Compact radio source 41. 9+58 in M82 as a young plerion
Journal Article · Sun Oct 31 23:00:00 EST 1982 · Sov. Astron. Lett. (Engl. Transl.); (United States) · OSTI ID:5984109
Are supernovae radio sources A search for radio emission from young supernova remnants
Journal Article · Tue Feb 28 23:00:00 EST 1978 · Astrophys. J.; (United States) · OSTI ID:5035922
Hard radiation by young pulsars as the cause of supernovae optical emission
Journal Article · Tue Dec 31 23:00:00 EST 1974 · Sov. Astron. AJ (Engl. Transl.); (United States) · OSTI ID:7265194

Related Subjects

640102* -- Astrophysics & Cosmology-- Stars & Quasi-Stellar
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
BRIGHTNESS
COSMIC RADIO SOURCES
ELECTROMAGNETIC RADIATION
ERUPTIVE VARIABLE STARS
OPTICAL PROPERTIES
PHYSICAL PROPERTIES
POWER
RADIATIONS
RADIOWAVE RADIATION
STARS
SUPERNOVA REMNANTS
SUPERNOVAE
VARIABLE STARS