'Host galaxy' diaporamas de présentation

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Yang Cui Friday July 26 th 2013 Committee: Gerald, Chris, Fabian, Art, Dan

Novel, Efficient Way to Study Origins of Globular Cluster Bimodality Calibration on MC Cluster NGC 1850a Application to GCs in the Sombrero Galaxy. Yang Cui Friday July 26 th 2013 Committee: Gerald, Chris, Fabian, Art, Dan. Presentation outline.

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Constraints on Secular Evolution from Star Clusters in Spirals and Lenticulars

Constraints on Secular Evolution from Star Clusters in Spirals and Lenticulars. Jean P. Brodie UCO/Lick Observatory University of California Santa Cruz. S tudy of A strophysics of G lobular clusters in E xtragalactic S ystems.

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Measuring Distances to Galaxies Using Water Vapor Megamasers

Measuring Distances to Galaxies Using Water Vapor Megamasers. Jim Braatz (NRAO). Measuring Distances to H 2 O Megamasers. NGC 4258. Thin -ring model: D = a -1 k 2/3 ? 4 /3 a = acceleration v = k r -1/2 ? = slope of sys features. ??. V r. 2V r 2??.

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Science by LCGT

Science by LCGT. Hideyuki Tagoshi (Osaka University). 2011/02/04 LCGT f2f meeting. Contents. Compact binary Coalescence (CBC) NS-NS Merger rate, event rate Parameter estimation accuracy Gravitational Collapse Pulsar Stochastic background. Detection of GW.

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Type Ia Supernovae as Probes of Dark Energy

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Simulations of Ly ? emission: fluorescence, cooling, galaxies

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The many mysteries of gamma-ray bursts R. Mochkovitch (IAP-Paris)

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Revisiting the Gamma-Ray Burst Classification in the Fermi Era

Revisiting the Gamma-Ray Burst Classification in the Fermi Era. ? ? ? ?????? / ?????? ???? ? ? ??? ???. Open Questions in GRB Physics (Zhang 2011). Classification Progenitor Central engine Ejecta composition Energy dissipation and particle acceleration mechanism

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The Newly-Discovered Remote Globular Cluster System of M31

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SN Ia Rates in the SNLS: Progress Report

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Observational Evidence of Creation

Observational Evidence of Creation. 2) The Universe is observed to be expanding (so in the past it was smaller). The Steady State Universe tried to get around this by supposing that new galaxies appear out of nowhere to fill the increasing volume

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Manuel Aravena, Jeff Wagg, Padelis Papadopoulos, Ilana Feain

A study of a ULIRG-to-QSO transition object: possibly another gas-rich/gas-poor merger and a serendipitous line detection. Manuel Aravena, Jeff Wagg, Padelis Papadopoulos, Ilana Feain. Outline. Introduction: the ULIRG to QSO evolutionary scenario

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Dr Katherine Inskip

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Riess, Strolger, Tonry et al astro-ph/0308185

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MAXIM: The Blackhole Imager

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1 st Doha International Astronomy Conference, 10-13 Feb 2013

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mpia.de/coevolution

Dynamical masses of lensed quasar host galaxies at z~2: Near Infrared Integral Field Spectroscopy with Laser Adaptive Optics Knud Jahnke 1 , Katherine J. Inskip 1 , Hans-Walter Rix 1 , Chien Y. Peng 2 1 MPI Astronomy, 2 Herzberg Inst. of Astrophysics. www.mpia.de/coevolution. M BH /M sun.

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STATISTICS

AMP: The GRB Afterglow Modeling Project Statistics and Extinction/Absorption Models Adam S. Trotter, Daniel E. Reichart & Andrew C. Foster University of North Carolina at Chapel Hill. ABSTRACT.

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