Parra, Rodrigo, Conway, John E., Diamond, Philip J., Thrall, Hannah, Lonsdale, Colin J., Lonsdale, Carol J., ...
We report the first detection at multiple radio wavelengths (13, 6 and 3.6 cm) of the compact sources within both nuclei of the Ultra Luminous Infra-Red Galaxy Arp 220. We present the radio spectra...
VLBI images of 49 radio supernovae in Arp 220 (2006)
Lonsdale, Colin J., Diamond, Philip J., Thrall, Hannah, Smith, Harding E., Lonsdale, Carol J.
We have used a very long baseline interferometry (VLBI) array at 18 cm wavelength to image the nucleus of the luminous IR galaxy Arp 220 at ∼1 pc linear resolution, with very high sensitivity. The...
VLBI Images of 49 Radio Supernovae in Arp 220 (2006)
Lonsdale, Colin J., Diamond, Philip J., Thrall, Hannah, Smith, Harding E., Lonsdale, Carol J.
We have used a Very Long Baseline Interferometry (VLBI) array at 18cm wavelength to image the nucleus of the luminous IR galaxy Arp 220 at ~1 pc linear resolution, and with very high sensitivity. The...
MERLIN monitoring of recent core-collapse supernovae (2005)
Argo, Megan, Beswick, Rob, Muxlow, Tom, Pedlar, Alan, Fenech, Danielle, Thrall, Hannah
The star formation rate (SFR) in starburst galaxies can be measured by many methods, one of which is through the supernova rate. Due to the heavy dust obscuration in these galaxies, searches for new...