A high-resolution H I study towards the supernova remnant Puppis A and its environments
We observed the supernova remnant Puppis A in the 21 cm line with the Australia Telescope Compact Array with the aim of determining the systemic velocity and, hence, the corresponding kinematic distance. For the compact, background sources in the field, we obtain absorption spectra by applying two m...
| Main Authors: | , , |
|---|---|
| Format: | Journal Article |
| Published: |
Oxford University Press
2017
|
| Online Access: | http://hdl.handle.net/20.500.11937/69074 |