Figure 1 – The left panel depicts the synchrotron emission at 1.4GHz, while the right panel depicts the 24-micron warm dust emission. Both panels are over plotted with the 1-3 GeV gamma ray emission.
Subscribe
Follow us on Twitter
More Posts About
protoplanetary disks astrophysics observations cosmology dark matter solar system simulations binary stars galaxies AAS theory Kepler transits galaxy evolution supernovae gravitational waves stars stellar evolution planetary science exoplanets spectroscopy astronomy black holes habitability Milky Way planet formation star formation dwarf galaxies AGN radio astronomy
Posts by Category
Our Sister Sites
(Organized under ScienceBites)
- Astrobitos (Astrobites in Spanish)
- Astropontos (Astrobites in Portugese)
- staryab (Farsi)
- ArAStrobites (Arabic)
- BiteScis (K12)
- Chembites
- Cogbites
- Envirobites
- Evobites
- ForensicBites
- Geobites
- Heritagebites
- ImmunoBites
- Nutribites
- Oceanbites
- OncoBites (Cancer)
- Particlebites
- PERbites (Physics Education Research)
- Reefbites
- Softbites
- astro[sound]bites