R. Dodson, K. Golap, J. Osborne, N. UdayaShankar, A. P. Rao
Published 2001-11-19Version 1
The observations of the supernova remnant G343.1-2.3 with the Mauritius Radio Telescope, the Australia Compact Array, and the Hobart Single dish are presented. With these more sensitive measurements the association with the pulsar PSR1706-44 becomes much more likely. The major points from the observations are presented.
Comments: 4 pages, 2 figures. IAU 199
Some arguments in support of the association of PSR B1706-44 with the supernova remnant G343.1-2.3
Hard X-Rays from the Galactic Nucleus: Present and Future Observations
New Observations and a New Interpretation of CO(3--2) in IRAS F10214+4724
