Abstract
The observation of intense gamma-ray line emission from the Orion complex, attributed by Bloemen et al. to de-excitation of cosmic-ray carbon and oxygen nuclei, has important implications for emission from Orion in the infrared and in high-energy gamma rays, and also for the theories of cosmic-ray origins. Some of these implications are briefly pointed out.
| Original language | English |
|---|---|
| Pages (from-to) | L29-L32 |
| Journal | Astrophysical Journal |
| Volume | 444 |
| Issue number | 1 PART 2 |
| DOIs | |
| State | Published - May 1 1995 |
Keywords
- Gamma rays: theory
- ISM: clouds
- ISM: individual (Orion Complex)