'Disk model' presentation slideshows

Towards a Scalable Database Service

Towards a Scalable Database Service. Samuel Madden MIT CSAIL. With Carlo Curino , Evan Jones, and Hari Balakrishnan. The Problem with Databases. Tend to proliferate inside organizations Many applications use DBs Tend to be given dedicated hardware Often not heavily utilized

750 views • 65 slides

Hyperbolic Geometry

3.31k views • 41 slides

Probing Accretion and Spacetime with Black Hole Binaries

Probing Accretion and Spacetime with Black Hole Binaries. Shane Davis IAS. Omer Blaes Ivan Hubeny Neal Turner Julian Krolik Jim Stone Shigenobu Hirose. Chris Done Mathew Middleton Marek Gierlinski Rebbeca Shafee Ramesh Narayan Jeff McClintock Ron Remillaird Li-Xin Li.

511 views • 39 slides

How do Black Hole Accretion Disks Radiate?

How do Black Hole Accretion Disks Radiate?. Shane Davis UCSB. Standard Accretion Picture. Issues Addressed in This Talk. How does the release of gravitational binding energy lead to ~ thermal radiation? Are thin disk ( a -disk) models sufficient to explain observations? (yes and no)

676 views • 39 slides

Probing Accretion and Spacetime with Black Hole Binaries

Probing Accretion and Spacetime with Black Hole Binaries. Shane Davis IAS. Omer Blaes Ivan Hubeny Neal Turner Julian Krolik Jim Stone Shigenobu Hirose. Chris Done Mathew Middleton Marek Gierlinski Rebbeca Shafee Ramesh Narayan Jeff McClintock Ron Remillaird Li-Xin Li.

541 views • 39 slides

Short Summary of the Mechanics of Wind Turbine

Short Summary of the Mechanics of Wind Turbine. Korn Saran-Yasoontorn Department of Civil Engineering University of Texas at Austin 8/7/02. Summarized from Wind energy explained: theory, design and application./ Manwell, J. F. / Chichester / 2002

674 views • 28 slides

Accretion onto Black Hole : Advection Dominated Flow

465 views • 26 slides

Thomas Henning and Dima Semenov

435 views • 25 slides

Shane Davis IAS

Probing Accretion and Spacetime with Black Hole Binaries. Shane Davis IAS. Omer Blaes Ivan Hubeny Neal Turner Julian Krolik Jim Stone Shigenobu Hirose. Chris Done Matthew Middleton Marek Gierlinski Rebecca Shafee Ramesh Narayan Jeff McClintock Ron Remillard Li-Xin Li.

383 views • 23 slides

ULXs and Evidence for Two IMBHs in M82

404 views • 22 slides

ULXs and Evidence for Two IMBHs in M82

235 views • 22 slides

Three-Dimensional Distribution of the Interstellar Dust in the Milky Way

Three-Dimensional Distribution of the Interstellar Dust in the Milky Way. Helong Guo ( ????helong_guo@mail.ynu.edu.cn ) Supervisor: Xiaowei Liu ? Bingqiu Chen Y unnan U niversity. Introduction.

201 views • 19 slides

Co-accreting disk/corona system in AGNs with double-peaked emission lines

Co-accreting disk/corona system in AGNs with double-peaked emission lines. XuYun. outline. 1.The properties of AGNs with double-peaked emission lines. 2.Our models. Co-accreting disk/corona system. 3.Other models. 4.Our research method. 5. Final result.

297 views • 17 slides

Locating Mass Loss

Locating Mass Loss. Numerical Modeling of Circumstellar Material in Binary Systems. Jennifer L. Hoffman University of Wisconsin-Madison Rice University. Where does mass loss occur in binary systems?. Binary evolution calculations often assume conservative mass transfer.

235 views • 15 slides

Disk Structure and Evolution (the so-called a model of disk viscosity)

Disk Structure and Evolution (the so-called a model of disk viscosity). Ge/Ay 133. Recapitulation of passive disk structure equations. I. Equation for hydrostatic equilibrium using only stellar gravity. For an ideal gas where c is the sound speed ( c 2 = R T).

314 views • 14 slides

Disk Structure and Evolution (the so-called a model of disk viscosity)

Disk Structure and Evolution (the so-called a model of disk viscosity). Ge/Ay 133. Recapitulation of passive disk structure equations. I. Equation for hydrostatic equilibrium using only stellar gravity. For an ideal gas where c is the sound speed ( c 2 = R T).

267 views • 14 slides

ANGULAR MOMENTUM TRANSPORT In T TAURI ACCRETION DISKS: WHERE IS THE DISK MRI-ACTIVE?

ANGULAR MOMENTUM TRANSPORT In T TAURI ACCRETION DISKS: WHERE IS THE DISK MRI-ACTIVE? Subhanjoy Mohanty (Imperial College London) Barbara Ercolano (University of Exeter) Neal Turner (JPL). I O H A. (Wardle 1999; Balbus & Terquem 2001; Kunz & Balbus 2004).

261 views • 13 slides

Spiral galaxies without Lambda Cold Dark Matter

Spiral galaxies without Lambda Cold Dark Matter. Piotr Skindzier Jagiellonian University 15 March, Moriond 2013 Suported by The National Science Centre grant nr. K/PBP/000391. O utline. Introduction Disk Model Vertical Gradient Summary. Introduction. Disk model.

277 views • 13 slides

The Standard Model of Low-Mass Star Formation Applied to Massive Stars Multi-wavelength Modelling

Rotationally flattened infalling envelope. The Standard Model of Low-Mass Star Formation Applied to Massive Stars Multi-wavelength Modelling. Katharine Johnston Collaborators: Eric Keto (CfA) Thomas Robitaille (CfA) Kenny Wood ( Univ. of St Andrews) Debra Shepherd (NRAO).

231 views • 10 slides

DVD Replication V/S DVD Duplication

When it comes to feeding some digital data in a digital versatile disk, people seldom confuse between digital versatile disk duplication and digital versatile disk replication. Read more.

17 views • 1 slides