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Evidence for Feedback in the IGM at High Redshift

Evidence for Feedback in the IGM at High Redshift

Evidence for Feedback in the IGM at High Redshift. Barlow (CIT), Becker (CIT), Boksenberg(IoA), Sargent (CIT), Simcoe (MIT), Rauch (OCIW). (based on QSO absorption line data from Keck HIRES, ESI and LRIS). How does the undisturbed IGM look ?.

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721 views • 60 slides
Guillem Anglada-Escude (1,2) Alan P. Boss(1) Alycia Weinberger (1) Ian Thompson (1)

Guillem Anglada-Escude (1,2) Alan P. Boss(1) Alycia Weinberger (1) Ian Thompson (1)

The C arnegie A strometric P lanet S earch and the role of ground based astrometry in the pre-Gaia era. Guillem Anglada-Escude (1,2) Alan P. Boss(1) Alycia Weinberger (1) Ian Thompson (1) (1)Carnegie Institution for Science (2) Institute for Astrophysics - University of Goettingen.

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518 views • 42 slides
A Charge-Based Magneto-Electric Test Procedure

A Charge-Based Magneto-Electric Test Procedure

A Charge-Based Magneto-Electric Test Procedure. Scott P. Chapman & Joseph T. Evans, Jr. Radiant Technologies, Inc. Aug 9, 2011 IWPMA 2011. Summary.

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497 views • 41 slides
Deriving the Physical Structure of High-mass Star Forming Regions

Deriving the Physical Structure of High-mass Star Forming Regions

Deriving the Physical Structure of High-mass Star Forming Regions. Yancy L. Shirley. Collaborators: Neal Evans, Kaisa Young, Dan Jaffe, Claudia Knez, & Jingwen Wu. May 2003. SF in the Milky Way. 10 11 stars in the Milky Way Evidence for SF throughout history of the galaxy (Gilmore 2001)

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480 views • 39 slides
Deriving the Physical Structure of High-mass Star Forming Regions

Deriving the Physical Structure of High-mass Star Forming Regions

Deriving the Physical Structure of High-mass Star Forming Regions. Yancy L. Shirley. Collaborators: Neal Evans, Kaisa Young, Dan Jaffe, Claudia Knez, & Jingwen Wu. May 2003. SF in the Milky Way. 10 11 stars in the Milky Way Evidence for SF throughout history of the galaxy (Gilmore 2001)

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399 views • 39 slides
Amplification of Magnetic Fields by Supernova-Driven Turbulence

Amplification of Magnetic Fields by Supernova-Driven Turbulence

Amplification of Magnetic Fields by Supernova-Driven Turbulence. Jongsoo Kim Korea Astronomy and Space Science Institute. Collaborators: Dinshaw Balsara (University of Notre Dame) Mordecai Mac Low (American Museum of Natural History). B-fields at intermediate z.

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471 views • 33 slides
IKI10230 Pengantar Organisasi Komputer Bab 7: Control Unit

IKI10230 Pengantar Organisasi Komputer Bab 7: Control Unit

IKI10230 Pengantar Organisasi Komputer Bab 7: Control Unit. Sumber : 1. Hamacher. Computer Organization , ed-5. 2. Materi kuliah CS152/1997, UCB. 28 Mei 2003 Bobby Nazief (nazief@cs.ui.ac.id) Qonita Shahab (niet@cs.ui.ac.id) bahan kuliah: http://www.cs.ui.ac.id/kuliah/iki10230/.

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443 views • 25 slides
Electron beam diagnostic methods

Electron beam diagnostic methods

Electron beam diagnostic methods. William S. Graves MIT-Bates Laboratory. Presented at 2003 ICFA S2E Workshop DESY-Zeuthen August, 2003. Experimental Methods. Hardware/software controls. Thermal emittance measurement using solenoid scan.

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434 views • 25 slides
WanKee Cho 1 , and Jongsoo Kim 2 Bon-Chul Koo 1

WanKee Cho 1 , and Jongsoo Kim 2 Bon-Chul Koo 1

Numerical Simulations on the Dynamical Evolution of Supernova Remnants near the Edge of Molecular Clouds. WanKee Cho 1 , and Jongsoo Kim 2 Bon-Chul Koo 1 1 Astronomy Division Department of Physics and Astronomy, Seoul National University 2 Korea Astronomy and Space Science Institute.

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350 views • 22 slides
Warm and Diffuse Gas and High Ionizzation Rate Near the Galactic Center

Warm and Diffuse Gas and High Ionizzation Rate Near the Galactic Center

Warm and Diffuse Gas and High Ionizzation Rate Near the Galactic Center from 140 pc West to 85 pc East of Sgr A*. Takeshi Oka , Chris MORONG, University of Chicago, Chicago Tom Geballe, Gemini Observatory, Hilo Nick Indriolo, Ben McCall, University of Illinois at Urbana-Champaign, Urbana

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255 views • 14 slides
Near-infrared interferometry of NGC 1068

Near-infrared interferometry of NGC 1068

Near-infrared interferometry of NGC 1068. Markus Wittkowski (ESO) Based on work (1998-2004) with R. Arsenault, Y. Balega, T. Beckert, W. J. Duschl, K.-H. Hofmann, P. Kervella, A. B. Men`shchikov, F. Paresce, D. Schertl, G. Weigelt. The immediate environment of the AGN. Uddy & Padovani.

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309 views • 14 slides

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