Shock Excited 1720 MHz Masers
1720 MHz OH masers have been detected towards a number of supernova remnants (SNRs) at the shock interface where the SNR slams into the interstellar medium. Models indicate that these masers are shock excited and can only be produced under tight constraints of the physical conditions. In particular,...
| Main Author: | |
|---|---|
| Other Authors: | |
| Format: | Others |
| Language: | en |
| Published: |
2009
|
| Subjects: | |
| Online Access: | De Witt, Aletha (2009) Shock Excited 1720 MHz Masers, University of South Africa, Pretoria, <http://hdl.handle.net/10500/1653> http://hdl.handle.net/10500/1653 |