The yellow hypergiant HR 5171 A: Resolving a massive interacting binary in the common envelope phase
Simulation Parameters and Results We performed nine simulations to test the sensitivity of our results to resolution, viscous stress-to-pressure ratio.
Infrared Spectroscopy of Neutron-Capture Elements in Planetary Nebulae N. C. Sterling & H. L. Dinerstein ABSTRACT We present results from an ongoing survey.
Great Debate on GRB Composition: A Case for Poynting Flux Dominated GRB Jets Bing Zhang Department of Physics and Astronomy University of Nevada, Las Vegas.
Asymptotic Giant Branch Stars
Astrophysical jets
Review Neutron Stars(NSs) and SNR (Crab Nebula…) and then on to BHs…
ASTEROSEISMOLOGY CoRoT session, January 13, 2007 Jadwiga Daszyńska-Daszkiewicz Instytut Astronomiczny, Uniwersytet Wrocławski.
High Energy Neutrino Astronomy Christian Spiering DESY Zeuthen TAUP 2001.
Dec. 11, 2007 1 Review Neutron Stars(NSs) and SNR (Crab Nebula…) and then on to BHs… SN-II produce a NS for massive stars in approx. range 8-15Msun; and.
EVOLUTION AND INTERNAL STRUCTURE OF RED GIANTS
