'Ir luminosity' presentation slideshows

Supernovae as resources of interstellar dust

Supernovae as resources of interstellar dust. Takaya Nozawa (IPMU, University of Tokyo). Collaborators; T. Kozasa , A. Habe (Hokkaido University) K. Maeda , K. Nomoto , M. Tanaka (IPMU) N. Tominaga (Konan Univ.), H. Umeda , I. Sakon (U.T.)

629 views • 48 slides

ESO

Recent Results on Reionization Chris Carilli (NRAO) Dakota/Berkeley,August 2011. CO intensity mapping during reionization: signal in 3 easy steps Recent results on f(HI) at z > 6 Gunn-Peterson overview Quasar near zones: a new tool J1120+0641 quasar at z=7.1: the Game Changer

445 views • 32 slides

Why are Some Brightest Cluster Galaxies Forming Stars?

303 views • 18 slides

Big Bang f(HI ) ~ 0

History of Baryons (mostly hydrogen). Big Bang f(HI ) ~ 0. Recombination. z = 1000 (0.4Myr). f(HI ) ~ 1. Reionization : Last phase of cosmic evolution to explore Bench-mark in cosmic structure formation indicating the formation of the first galaxies. Redshift. Reionization.

297 views • 14 slides

WP6200 : Padova Scientific Activities

181 views • 9 slides