'Mass loss rates' presentation slideshows

Circumstellar interaction in Type II SNe Evidence for CSI in different Type II SNe.

Circumstellar interaction in Type II SNe Evidence for CSI in different Type II SNe. CSI as a shock physics lab The ring collision of SN 1987A. How does it fit in?. SN 1993J. Radio: Synchrotron spectrum Wavelength dependent turn-on of emission VLBI imaging of SN 1993J and SN 1986J.

665 views • 50 slides

Astronomy 535 Stellar Structure Evolution

534 views • 31 slides

Radio Science and PILOT

Radio Science and PILOT. Tony Wong ATNF/UNSW PILOT Workshop 26 March 2003. New Synergies. PILOT: 2m, 1-30 ? m (10-300 THz). Starlight, thermal dust continuum, recombination lines, excited H 2 , PAH features.

190 views • 6 slides