Astronomy
Multiwavelength observations of_na_st1_(wr122)_equatorial_mass_loss_and_x_rays_from_an_interacting_wolf_rayet_binary
WR_talk_FWS_volendam2014.pptx
20 April 2001AAO Workshop1 Optical & IR Interferometry Bill Tango School of Physics University of Sydney.
.... Chepelare, Bulgaria, June 1-4, 2010 VII Bulgarian-Serbian Astronomical Conference ASTROINFORMATICS Astroinformatics for the Flare Stars in Stellar.
WHERE IS FLUORINE? By: Ann Dyer, Samantha Sullivan, and Isaac Richter.
Observational techniques meeting #9. Spectroscopy.
SLAC, October 7 th 2004 1 Multifrequency Strategies for the Identification of Gamma-Ray Sources Reshmi Mukherjee, Jules Halpern Marcus Ziegler Santa Cruz.
Goal: To understand the post main sequence evolutions of the most massive stars Objectives: 1)To learn about Eta Carinae and LBVs 2)To learn about what.
WESTERLUND 1 : A SUPER STAR CLUSTER IN THE MILKY WAY
Jamie Holder and Gernot Maier University of Delaware/ McGill University
Gamma ray bursts from binary black holes Agnieszka Janiuk Center for Theoretical Physics, Polish Academy of Sciences, Warsaw Collaboration: Szymon Charzyński.
