Hello!. Ajit Kembhavi IUCAA, Pune Galaxies Near and Far Galaxy Morphology, SuperMassive Black Holes and all that Sudhanshu Barway Yogesh Wadadekar Vinu.
Close encounters between stars and Massive Black Holes Clovis Hopman Weizmann Institute of Science Israel Advisor: Tal Alexander.
Dynamics of Quantum- Degenerate Gases at Finite Temperature Brian Jackson Inauguration meeting and Lev Pitaevskii’s Birthday: Trento, March 14-15 University.
Did Dark Matter Annihilations Reionize The Universe? Dan Hooper Fermilab Theoretical Astrophysics Group FNAL Particle Astrophysics Seminar June 1, 2009.
Spectacular Shells in the Host Galaxy of the QSO MC2 1635+119
Fig. 2 Coordinate system. The subscripts i, p, and d refer to the intruder, particle and disk respectively. (a), (b) Side and top view, respectively. (c)
The KAT/SKA project and Related Research Catherine Cress (UKZN/KAT/UWC)
Maxime KUBRYK, IAP, Ph.D student advisors: Nikos PRANTZOS, IAP Lia ATHANASSOULA, OAMP LIA-ORIGINS, May 2012.
Fig. 2 Coordinate system .
From the very first stars to z~6 supermassive black holes
Asymmetric Neutrino Reaction in Magnetized Proto-Neutron Stars in fully Relativistic Approach Nuclear Matter ⇒ RMF Approach Different Mean-Field for p,
Wide Field Imagers in Space and the Cluster Forbidden Zone Megan Donahue Space Telescope Science Institute Acknowledgements to: Greg Aldering (LBL) and.