'Cooling time' presentation slideshows

Photons and Neutrinos Originating from Accelerated Protons in GRBs

Photons and Neutrinos Originating from Accelerated Protons in GRBs. Katsuaki ASANO (National Astronomical Observatory of Japan). Collaborators: S.Inoue, S.Nagataki, F.Takahara. Abstract.

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What goes up and down the stairs without moving?

You throw away the outside and cook the inside. Then you eat the outside and throw away the inside. What did you eat?. What goes up and down the stairs without moving?.

565 views • 45 slides

INTRODUZIONE A: Aloni radio Ammassi di galassie con e senza cool core

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What is the Fate of the Cooling Gas?

What is the Fate of the Cooling Gas?. G. M. Voit. The Agenda. Clusters bear the signature of galaxy formation Entropy is key property Global properties governed by cooling & feedback Core entropy distribution offers clues to feedback mechanism. Luminosity-Temperature Relation.

429 views • 29 slides

p-bar target

Atomic Physics. FAIR Baseline Layout. SIS 100. SIS18 Upgrade. p-linac. SIS 300. SIS100 SIS300. p-linac. HADES & CBM. PANDA. SuperFRS. Unilac. Antiproton Prod. Target. HESR. HESR. High Energy Exp. Super- FRS. Plasma Phys. Low Energy Exp. p-bar target. Atomic Phys.

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Current standing of the undulator based ILC positron source

Current standing of the undulator based ILC positron source. Wei Gai AWLC 14 FNAL, May 13 2014. ILC TDR positron source location. Target for e+ production. 147 m helical undulator for photon production. Optical Matching Device for e+ capture. PBSTR 400MeV-5GeV. PPA (125-400MeV).

387 views • 26 slides

Elizabeth Blanton University of Virginia

Chandra Observations of Radio Sources in Clusters: Impact on the ICM and Tracers of High-z Systems. Elizabeth Blanton University of Virginia. Collaborators: C. L. Sarazin, B. R. McNamara, N. Soker, M. W. Wise, T. E. Clarke, D. J. Helfand, M. D. Gregg, R. H. Becker, R. L. White.

384 views • 24 slides

Determining the location of the GeV emitting zone in fast, bright blazars

Determining the location of the GeV emitting zone in fast, bright blazars. Amanda Dotson, UMBC Markos Georganopoulos (advisor), UMBC/GSFC Eileen Meyer, STScI Kevin McCann, UMBC. AAS Meeting, Washington DC January 2014. The Issue At Hand.

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335 views • 22 slides

Igneous Rocks Rocks & Minerals Notes: Page 7

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Results with ISCOOL a new Radio Frequency Quadrupole Cooler and Buncher at ISOLDE

329 views • 20 slides

Results with ISCOOL a new Radio Frequency Quadrupole Cooler and Buncher at ISOLDE

315 views • 19 slides

Ultrafast dynamics in ZnO/ZnMgO multiple quantum wells (MQW)

Ultrafast dynamics in ZnO/ZnMgO multiple quantum wells (MQW). Speaker: Ho-Jei Ton Advisor: Jia-Hon Lin. Outline. Introduction Experimental sample and technique Experimental results and discussion Summary. Introduction.

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Chandra observations of the central region of Abell 3112

Chandra observations of the central region of Abell 3112. M. Takizawa (Yamagata Univ.) C. L. Sarazin, E. L. Blanton (Univ. of Virginia) G. B. Taylor (NRAO). Introduction. We have a lot of unsolved problems about the cluster center. Radiative cooling (cooling flows) Where is cold gas ?

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Gore High School Year 13

142 views • 14 slides

Frenk, Bauch Cole, Lacey

Wang 2000; Chandra obs of NGC4632. Frenk, Bauch Cole, Lacey. Hydrostatic Equilirium of Gas in DM potential wells. Radiative Cooling: I Collisional Excitation. v. T ~ 10 5 - 10 8 K. j. g. i. v. hv=E ij. Condition: En. of Elettrons E ? KT > D E lu. Collision rate.

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Forced Convection of Ramen Noodles by Human Expiration

249 views • 5 slides

Radiation Safety Considerations

Radiation Safety Considerations. Ambient dose equivalent rate at a transverse distance of 50cm to the beam axis:. cooling times in hours. at the dump: < 200 mrem/h. average in the aisle: < 1 mrem/h. Radiation Safety Considerations. Cooling time scaling factors:.

199 views • 4 slides

biscuit manufacturing process

biscuit process , biscuit manufacturing

5.48k views • 1 slides