Controls the re-ionization of the Universe. Determines the phase structure of the Interstellar Medium ... Kurk, Pentericci, R ttgering, Miley & Heckman: ...
During the mid-90's, with improved instrumentation, the commissioning of the 8-m ... VLA, ultra deep HDF-N ( Merlin, WSRT) JCMT SCUBA sub-mm maps of HDF-N ...
VLT+NACO monitoring of 14 ULIRGs out to D ~ 300 Mpc. Historical SN in NGC 7714 Found in archival UKIRT K image from Sep 1998. Optimal Image Subtraction Allard ...
... (large lookback times) forming via mergers Sgr dwarf elliptical merging with Milky Way The Local Group -- Andromeda (M31) and Milky Way Artists concept ...
Dust vs non-dusty SEDs. Extinction Laws. PAHs in NGC7331. PAHs in Starburst M82. PAHs vs [O/H] ... One after that: Levenson et al. 2005, ApJ, 618, 167: ...
Core-collapse SNe (CCSNe) generate/liberate the bulk of the ... Can serve as probes of extinction and ISM. CCSNe blast wave probes progenitor mass-loss history. ...
Need much better sensitivity to get near Cas A power, or to observe many more modest starbursts ... needs lots of long(ish) baselines, and frequencies above a ...
Identify starburst galaxies, derive luminosity functions, lifetimes and masses. Examine the link between starburst and ... Study the starburst - AGN connection ...
3C Radio Galaxies at 60mm with IRAS. Only ~30% of 3CR radio galaxies at z 0.5. were detected by IRAS at 60mm. Spitzer/MIPS observations of complete samples of ...
deep Ha, UV imaging of volume-complete 11 Mpc samples - Spitzer followup proposed ... Ha imaging followup of Arecibo ALFALFA HI survey. Fourth Generation: blind ...
Use calculated tQ and measured f to find n ?(Lpeak) And you get. Simulation ... Getting Quasar Creation Rate n. ? f = the comoving number density of quasars in ?log L ...
Lecture 3 The role of stars in AGN Evidence for stars in the nuclear regions of type-2 AGN Photoionization models for starbursts Type IIn supernovae: variability
The other side of galaxy formation: radio line and continuum ... Extreme gas rich galaxies without extreme starbursts. Gas depletion timescales 5 x108 yrs ...
Comparable SFR at high z in dusty starbursts ('submm gal') as ... Optical phot z. Radio phot z: (1 z) propto T_D. 20K. 60K. Z_rad, Z_opt(2) Z_opt (1) COSBO 7 ...
The solar wind interacts with the Earth, providing a way for the ... Some galaxies even appear to be undergoing 'starbursts', dominated by young, massive stars. ...
SCUBA gals, starbursts, AGN) ... Old Stellar Populations at Early Epochs Ages and metallicities of stellar ... Old stellar populations: determine age ...
How are starbursts, low surface brightness galaxies different? Timescales ... value depends on corrections for dust obscuration, surface-brightness dimming ...
Dust absorbs the radiation produced by starbursts or AGN ... sufficient to blow away. all of the gas in a galaxy ... If L LM, AGN can blow dusty gas out of. its ...
Found in nearby star-forming galaxies, starbursts, and AGNs. ... Structures of exotic star-formation in outer galaxies. ... star-forming galaxy, hosting a low ...
ISO results show spectroscopic discrimination of starbursts and AGN achievable in infrared. Hubble, Keck results show Universe full of galaxies at z 3 ...
Bell Work: 10/20/14 Write the answer and explain why the answer you chose is correct (justify your answer). What type of rock is most likely formed by process 3?
As the boy went back to his family s farm laughing about the funny trick he played, ... The school day was ending, but Angie wanted to keep coloring, ...
Bell Work: 10/20/14 Write the answer and explain why the answer you chose is correct (justify your answer). Have your notebook open to your Paper Plate Rock Cycle.
Tenth Summer Synthesis Imaging Workshop. University of New ... Brighten and deflect. Gomez et al. 2000. 26. Where Most X-rays & ?-rays Are Emitted. clouds ...
Ultraluminous Infrared Galaxies (ULIRGs) Discovered by IRAS in mid 80's ... Key Phase in Growth of Elliptical Galaxies and Massive BHs? Chapman et al. 2004 ...
WHIM Backlight Scaling relation fudge factor Point source contaminant Cooling problem get-out clause AGN/GALAXY COEVOLUTION Kirpal Nandra Imperial College London
Chandra Deep Field-North data. Source Redshifts. Diversity of X-ray selected sources ... Moderately deep Chandra surveys reported little overlap with the submm source ...
Theme The Search for Meaning What is a Theme? Theme: Life lesson, meaning, moral, or message about life or human nature that is communicated by a literary work.
Supervisor: Anja C. Andersen. Dust in Young Galaxies. 2. The code. Radiative transfer ... Dust Extinction in Starburst Galaxies at z = 3 6. Dust Creation in ...
The SWIRE Spitzer survey has detected by far the largest set of Sub-Millimeter ... Chapman, Blain, Smail, Ivison 2005. SCUBA(-MAMBO) census of high-z ULIRGs ...
Although one expects some correlation between bright sources in mid-IR ... Deep radio surveys in many Spitzer fields ... 900h mapping most Spitzer survey fields ...
Some galaxies show evidence of a recent and transient increase in ... The objects fainter than 16.m5 are, as a rule, worthless for statistical investigation. ...
Title: Introduction to the Mole and Molar Mass Author: S. Stevens Last modified by: Gloria Kandrick Created Date: 9/18/2004 6:36:17 PM Document presentation format
Molecular Gas, Dense Molecular Gas and the Star Formation Rate in Galaxies (near and far) P. Solomon Molecular Gas Mass as traced by CO emission and the star ...
with input from Heald, Anderson, Beck. p. 15. Key Drivers. 100 z ~ 6 radio galaxies ... Galactic radio sources Marijke Haverkorn / Glenn White. p. 25 ...
present-day stars, it would be logical. to expect to detect a large ... 4 Populations: Spiral (M51), Starburst (M82), AGN1 (Elvis et al. 94) & AGN2 (Circinus) ...
Introduction to the Mole and Molar Mass Revised 9/05/06 Purpose At the completion of this unit students will Have a conceptual understanding of the mole as the method ...