DocumentCode
3041024
Title
Radio spectrum variations in supernova remnants
Author
Leahy, Denis ; Wenwu, Tian
Author_Institution
Dept. of Phys. & Astron., Univ. of Calgary, Calgary, AB
fYear
2009
fDate
15-18 Feb. 2009
Firstpage
1
Lastpage
4
Abstract
Supernova remnants are prominent sources of astronomical radio emission within our Galaxy. The mechanism is synchrotron radiation from relativistic electrons and the observed spectrum depends on the relativistic electron spectrum and propagation effects from the source to the observer. Here the electron spectrum and radio absorption effects are discussed and compared with recent observations of galactic supernova remnants.
Keywords
astronomical spectra; astrophysical radiation mechanisms; radiosources (astronomical); supernova remnants; astronomical radio emission sources; galactic supernova remnants; propagation effects; radio absorption effects; radio spectrum variations; relativistic electron spectrum; synchrotron radiation; Acceleration; Astronomy; Electric shock; Electromagnetic wave absorption; Electron emission; Frequency; Magnetic fields; Physics; Space technology; Synchrotrons;
fLanguage
English
Publisher
ieee
Conference_Titel
Antenna Technology and Applied Electromagnetics and the Canadian Radio Science Meeting, 2009. ANTEM/URSI 2009. 13th International Symposium on
Conference_Location
Banff, AB
Print_ISBN
978-1-4244-2979-0
Electronic_ISBN
978-1-4244-2980-6
Type
conf
DOI
10.1109/ANTEMURSI.2009.4805087
Filename
4805087
Link To Document