'Star forming galaxies' presentation slideshows

MIPS Observations of Galaxies, Near and Far

754 views • 68 slides

FORMATION AND EVOLUTION OF GALAXIES FROM INFRARED AND RADIO SURVEYS

FORMATION AND EVOLUTION OF GALAXIES FROM INFRARED AND RADIO SURVEYS. Carlotta Gruppioni (INAF-OABO) Bologna 1 Ottobre 2007. SUMMARY. Advantages of IR and radio IR & radio emission from galaxies Early galaxy evolution results in IR and radio: source counts & luminosity function

783 views • 56 slides

Downsizing & Galaxy Formation

Downsizing & Galaxy Formation. P. McCarthy OCIW. Gemini Deep Deep Survey Team. 2 nd Mitchell Symposium - April 2006. How are Galaxies Formed?. Monolithic Collapse ala ELS. Hierarchical Assembly . The Hierarchical Merger Tree. -----------------. Z = 3. ---------------. Z = 1.

746 views • 49 slides

Current Topics

Current Topics. Lyman Break Galaxies Dr Elizabeth Stanway (E.R.Stanway@Bristol.ac.uk). Topic Summary. Star Forming Galaxies and the Lyman- ? Line Lyman Break Galaxies at z <4 Lyman Break Galaxies at z >4 Lyman Break Galaxies at z>7 Reionisation, SFH and Luminosity Functions.

517 views • 40 slides

HI at moderate redshifts Philip Lah Science with MIRA workshop

509 views • 40 slides

AGN / Starbursts in the very dusty systems in Bootes

AGN / Starbursts in the very dusty systems in Bootes. Kate Brand + the Bootes team NOAO Lijiang, August 2005. The Importance of ULIRGS. ULIRGs have L bol >10 12 L o and contribute significantly to the total energy budget of the Universe.

276 views • 20 slides

How do galaxies accrete their mass? Quiescent and star - forming massive galaxies at high z

How do galaxies accrete their mass? Quiescent and star - forming massive galaxies at high z. Paola Santini. Osservatorio Astronomico di Roma. THE ORIGIN OF GALAXIES: LESSONS FROM THE DISTANT UNIVERSE Obergurgl, 12 - 17 December 2009. z ? 2 : major phase in the assembly of massive galaxies.

323 views • 18 slides

Discovery of a multiply-imaged Ly- ? galaxy at the redshift of a SCUBA galaxy at z=2.56

Discovery of a multiply-imaged Ly- ? galaxy at the redshift of a SCUBA galaxy at z=2.56. Helmut Dannerbauer (MPIA) in collaboration with M.D. Lehnert (OBSPM) L. Douglas (OBSPM), J.-P. Kneib (Marseille), N. Nesvadba (OBSPM), J. Richard (Caltech), C. Tapken (MPIA). H ? of field of Abell 1835.

295 views • 16 slides

How do galaxies accrete their mass? Quiescent and star - forming massive galaxies at high z

315 views • 16 slides

AGN / Starbursts in the very dusty systems in Bootes

AGN / Starbursts in the very dusty systems in Bootes. Kate Brand + the Bootes team NOAO Lijiang, August 2005. The Importance of ULIRGS. ULIRGs have L bol >10 12 L o and contribute significantly to the total energy budget of the Universe.

258 views • 15 slides

Migration of Nearby Spirals

Migration of Nearby Spirals. AGN feedback or Environmental effects?. Tom Hughes. Supervisors: Luca Cortese, Jonathan Davies astro-ph:0903.3574. Red. Blue. Wyder et al, 2007. Borch et al, 2006. Migration of galaxies. Blue Red What drives the migration?.

226 views • 11 slides

Gamma Ray Burst Discoveries with the Swift Mission

Gamma Ray Burst Discoveries with the Swift Mission. Neil Gehrels NASA/GSFC N 2 PS 2 - GWU June 16, 2008. UVOT. XRT. BAT. BAT. XRT. Swift Mission NASA MIDEX. 3 instruments - BAT, ? -rays 15-350 keV - XRT, X-rays, 0.2-10 keV - UVOT, opt, 170-650 nm

200 views • 5 slides

Compact Star Clusters in HII Galaxies

97 views • 1 slides

Astrophysical Journal, 2004, 608, 768 Abstract

139 views • 1 slides