Image:AGN Jet Synchro-Spectrum.png
From Wikipedia, the free encyclopedia
AGN_Jet_Synchro-Spectrum.png (378 × 274 pixel, file size: 37 KB, MIME type: image/png)
A sketch of the spectrum of a non-thermal synchrotron source. On the left the flux density rises in the optically thick region. After the peak frequency the spectrum falls, with an additional break indicating very short lifetimes for high energy electrons.
Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.2 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts.
Subject to disclaimers.
File history
Legend: (cur) = this is the current file, (del) = delete
this old version, (rev) = revert to this old version.
Click on date to download the file or see the image uploaded on that date.
- (del) (cur) 19:51, 18 April 2006 . . Mrbrak (Talk | contribs) . . 378×274 (37,565 bytes) (A sketch of the spectrum of a non-thermal synchrotron source. From Nasa.)
- (del) (rev) 19:34, 18 April 2006 . . Mrbrak (Talk | contribs) . . 378×274 (37,565 bytes) (Synchrotron Spectrum. A sketch of the synchrotron spectrum. From Nasa.)
- (del) (rev) 19:29, 18 April 2006 . . Mrbrak (Talk | contribs) . . 378×274 (37,565 bytes) (Synchrotron Spectrum. A diagram of the synchrotron spectrum. From Nasa.)
- (del) (rev) 06:51, 1 November 2004 . . Mrbrak (Talk | contribs) . . 450×334 (25,412 bytes) (A sketch of the spectrum of a non-thermal synchrotron source. On the left the flux density rises in the optically thick region. After the peak frequency the spectrum falls, with an additional break indicating very short lifetimes for high energy electrons)
- Edit this file using an external application
See the setup instructions for more information.