Blazars @ -ray and other frequencies P. Giommi Agenzia Spaziale Italiana.
LECTURE 27, DECEMBER 9, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT [email protected] 1ASTR 101-3, FALL 2010.
Agn
Detection of Light
11 July 20036dF workshop1 Radio sources in the 6dFGS Tom Mauch & Elaine Sadler University of Sydney ‘Main survey’ science: Faint end of radio luminosity.
CO J =1-0 + J =3-2 map (Oka+ 1999, 2007) Galactic Center Kunihiko Tanaka (1), Tomoharu Oka (1), Shinji Matsumura (1), Kazuhisa Kamegai (2), Makoto Nagai.
ASTR100 (Spring 2008) Introduction to Astronomy Galaxy Evolution & AGN Prof. D.C. Richardson Sections 0101-0106.
Panorama of the Universe: Daily all-sky surveys with the SKA John D. Bunton, CSIRO TIP, Ronald D. Ekers, CSIRO ATNF and Elaine M. Sadler, University of.
Instituto de Astrofísica de Andalucía – C.S.I.C Research Institute of the Consejo Superior de Investigaciones Cientificas Main activities devoted to Astrophysics.
15.3 Galaxy Evolution Our Goals for Learning How do we observe the life histories of galaxies? How did galaxies form? Why do galaxies differ?
NUclei of GAlaxies: First results of NUGA Santiago GARCIA BURILLO ([email protected]) Observatorio Astronómico Nacional (OAN) The NUGA project People involved.
Galaxy Morphology The Tuning Fork that Blossomed into a Lemon Lance Simms MASS Talk 9/8/08.
