13 March 201313rd MAXI Symposium Be Be. Talk Outline 1.Introduction to Be stars 2.Decretion vs. accretion 3.Interactions in binaries 4.Concluding remarks.
Brooks International Speakers Bureau Exclusively Represents Faisal Hoque, BTM CEO and Keynote Speaker
Faisal Hoque - Author of "The Power of Convergence" and Keynote Speaker Represented by Brooks International
intro[1]
Star formation at high redshift (2 < z < 7) Methods for deriving star formation rates UV continuum = ionizing photons (dust obscuration?) Ly = ionizing.
Selected topics on Cosmic Magnetic fields Huirong Yan KIAA-PKU hryan.
1 . The Stellar Populations of NGC5128
Radio Galaxy workshop: so what?
Star formation at high redshift (2 < z < 7)