Shock Excited 1720 MHz Masers

Shock Excited 1720 MHz Masers

Show other versions (1)

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,...

Full description

Bibliographic Details
Main Author: De Witt, Aletha
Other Authors: Smits, D. P.
Format: Others
Language:en
Published: 2009
Subjects:
Supernova remnants
Star formation
Shock waves
Pre-main sequence
Molecules
Mass loss
Masers
Jets and outflows
Herbig Haro objects
Clouds
621.381336
Herbig-Haro objects (Astronomy)
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

Internet

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

Similar Items