Accretion disc

Results: 160



#Item
1Accretion Physics inStellar-Mass Compact Objects

Accretion Physics inStellar-Mass Compact Objects

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Source URL: ixo.gsfc.nasa.gov

Language: English - Date: 2008-12-29 13:25:37
2Cool star studies with IXO Marc Audard (University of Geneva)  ESA IXO Conference, Munich 17­19 September 2008

Cool star studies with IXO Marc Audard (University of Geneva) ESA IXO Conference, Munich 17­19 September 2008

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Source URL: ixo.gsfc.nasa.gov

Language: English - Date: 2008-12-29 13:26:10
3Pushing IXO to the Extreme Phil Uttley University of Southampton Black hole power: key questions

Pushing IXO to the Extreme Phil Uttley University of Southampton Black hole power: key questions

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Source URL: ixo.gsfc.nasa.gov

Language: English - Date: 2008-12-29 13:26:06
4A&A 560, A56DOI: Astronomy & Astrophysics

A&A 560, A56DOI: Astronomy & Astrophysics

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Source URL: cds.aanda.org

Language: English
5Vol 444 | 16 November 2006 | doi:nature05323  LETTERS Hydrodynamic turbulence cannot transport angular momentum effectively in astrophysical disks Hantao Ji1, Michael Burin1{, Ethan Schartman1 & Jeremy Goodman1

Vol 444 | 16 November 2006 | doi:nature05323 LETTERS Hydrodynamic turbulence cannot transport angular momentum effectively in astrophysical disks Hantao Ji1, Michael Burin1{, Ethan Schartman1 & Jeremy Goodman1

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Source URL: mri.pppl.gov

Language: English - Date: 2006-11-15 15:09:40
6Summary of Monday sessions Marek Sikora Kraków, April 2015  Andrew Hamilton:

Summary of Monday sessions Marek Sikora Kraków, April 2015 Andrew Hamilton:

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Source URL: www.oa.uj.edu.pl

Language: English - Date: 2015-04-22 01:30:12
7Angular momentum transport in astrophysics and in the lab Hantao Ji and Steven Balbus For evolving astrophysical accretion disks to concentrate their mass and still conserve angular momentum, turbulent flows are crucial.

Angular momentum transport in astrophysics and in the lab Hantao Ji and Steven Balbus For evolving astrophysical accretion disks to concentrate their mass and still conserve angular momentum, turbulent flows are crucial.

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Source URL: w3.pppl.gov

Language: English - Date: 2013-07-31 20:19:08
8Relativistic Jet Properties of GeV AGNs. II. Correlations among Jet, Disk, and Broad Line Region Jin 1 Zhang ,

Relativistic Jet Properties of GeV AGNs. II. Correlations among Jet, Disk, and Broad Line Region Jin 1 Zhang ,

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Source URL: www.oa.uj.edu.pl

Language: English - Date: 2015-05-08 02:56:49
9RAPID COMMUNICATIONS  PHYSICAL REVIEW E 89, RNonlinear stability of laboratory quasi-Keplerian flows E. M. Edlund and H. Ji

RAPID COMMUNICATIONS PHYSICAL REVIEW E 89, RNonlinear stability of laboratory quasi-Keplerian flows E. M. Edlund and H. Ji

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Source URL: w3.pppl.gov

Language: English - Date: 2014-03-01 08:42:32
10Mon. Not. R. Astron. Soc. 325, L1–L5Magnetorotational instability in a rotating liquid metal annulus Hantao Ji,1P Jeremy Goodman2 and Akira Kageyama1,3 1

Mon. Not. R. Astron. Soc. 325, L1–L5Magnetorotational instability in a rotating liquid metal annulus Hantao Ji,1P Jeremy Goodman2 and Akira Kageyama1,3 1

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Source URL: w3.pppl.gov

Language: English - Date: 2001-08-01 10:53:15