ar X iv : 1 41 0 . 79 58 v 1 [ as tr o - ph . C O ] 2 9 O ct 2 01 4 Observing the Inflationary Reheating

ar X iv : 0 70 5 . 31 41 v 1 [ as tr o - ph ] 2 2 M ay 2 00 7 The SARG Planet Search

ar X iv : 0 81 0 . 43 71 v 1 [ as tr o - ph ] 2 4 O ct 2 00 8 Welcome back , Polaris the Cepheid

For about 100 years the amplitude of the 4 d pulsation in Polaris has decreased. We present new results showing a significant increase in the amplitude based on 4.5 years of continuous monitoring from the ground and with two satellite missions.

ar X iv : h ep - p h / 02 10 05 0 v 1 3 O ct 2 00 2 1 20 + years of Inflation

In this talk I will review the present status of inflationary cosmology and its emergence as the basic paradigm behind the Standard Cosmological Model, with parameters determined today at better than 10% level from CMB and LSS observations. I will also discuss the recent theoretical developments on the process of reheating after inflation and model building based on string theory and D-branes.

ar X iv : 0 70 5 . 32 58 v 1 [ as tr o - ph ] 2 2 M ay 2 00 7 Disks around Young Binary Stars

ar X iv : 0 71 0 . 33 59 v 1 [ as tr o - ph ] 1 7 O ct 2 00 7 Generation of Magnetic Field by Combined Action of Turbulence and Shear

T. A. Yousef, T. Heinemann, A. A. Schekochihin, N. Kleeorin, I. Rogachevskii, A. B. Iskakov, 2, 5 S. C. Cowley, 2 and J. C. McWilliams DAMTP, University of Cambridge, Cambridge CB3 0WA, United Kingdom Plasma Physics Group, Blackett Laboratory, Imperial College, London SW7 2AZ, United Kingdom Department of Mechanical Engineering, The Ben-Gurion University of the Negev, P. O. Box 653, Beer-Sheva ...