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
binary stars accretion astrophysics star formation theory galaxy evolution protoplanetary disks transits AAS solar system galaxies spectroscopy black holes habitability astronomy planetary science gravitational waves AGN Kepler supernovae simulations planet formation cosmology radio astronomy stars dark matter observations exoplanets astronomical methods stellar evolution
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