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.
Stellar Winds and Mass Loss Brian Baptista. Summary Observations of mass loss Mass loss parameters for different types of stars Winds colliding with the.
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
