These tools will no longer be maintained as of December 31, 2024. Archived website can be found here. PubMed4Hh GitHub repository can be found here. Contact NLM Customer Service if you have questions.


BIOMARKERS

Molecular Biopsy of Human Tumors

- a resource for Precision Medicine *

100 related articles for article (PubMed ID: 17731145)

  • 1. Keplerian complexity: numerical simulations of accretion disk transport.
    Hawley JF
    Science; 1995 Sep; 269(5229):1365-70. PubMed ID: 17731145
    [TBL] [Abstract][Full Text] [Related]  

  • 2. Hydrodynamic turbulence cannot transport angular momentum effectively in astrophysical disks.
    Ji H; Burin M; Schartman E; Goodman J
    Nature; 2006 Nov; 444(7117):343-6. PubMed ID: 17108959
    [TBL] [Abstract][Full Text] [Related]  

  • 3. Stability and angular-momentum transport of fluid flows between corotating cylinders.
    Avila M
    Phys Rev Lett; 2012 Mar; 108(12):124501. PubMed ID: 22540587
    [TBL] [Abstract][Full Text] [Related]  

  • 4. Development of a Couette-Taylor flow device with active minimization of secondary circulation.
    Schartman E; Ji H; Burin MJ
    Rev Sci Instrum; 2009 Feb; 80(2):024501. PubMed ID: 19256666
    [TBL] [Abstract][Full Text] [Related]  

  • 5. Angular Momentum Transport by Keplerian Turbulence in Liquid Metals.
    Vernet M; Fauve S; Gissinger C
    Phys Rev Lett; 2022 Aug; 129(7):074501. PubMed ID: 36018687
    [TBL] [Abstract][Full Text] [Related]  

  • 6. The magnetic nature of disk accretion onto black holes.
    Miller JM; Raymond J; Fabian A; Steeghs D; Homan J; Reynolds C; van der Klis M; Wijnands R
    Nature; 2006 Jun; 441(7096):953-5. PubMed ID: 16791188
    [TBL] [Abstract][Full Text] [Related]  

  • 7. Counterrotating galaxies and accretion disks.
    Lovelace RV
    Ann N Y Acad Sci; 1998 Dec; 867():217-28. PubMed ID: 12088041
    [TBL] [Abstract][Full Text] [Related]  

  • 8. High-growth-rate magnetohydrodynamic instability in differentially rotating compressible flow.
    Sharma M
    Phys Rev E Stat Nonlin Soft Matter Phys; 2010 Sep; 82(3 Pt 2):037302. PubMed ID: 21230216
    [TBL] [Abstract][Full Text] [Related]  

  • 9. Emergence of high peaks in the axial velocity for an ideal magnetohydrodynamic disk configuration.
    Montani G; Carlevaro N
    Phys Rev E Stat Nonlin Soft Matter Phys; 2010 Aug; 82(2 Pt 2):025402. PubMed ID: 20866868
    [TBL] [Abstract][Full Text] [Related]  

  • 10. Binary black-hole mergers in magnetized disks: simulations in full general relativity.
    Farris BD; Gold R; Paschalidis V; Etienne ZB; Shapiro SL
    Phys Rev Lett; 2012 Nov; 109(22):221102. PubMed ID: 23368111
    [TBL] [Abstract][Full Text] [Related]  

  • 11. Angular momentum transport in thin accretion disks and intermittent accretion.
    Coppi B; Coppi PS
    Phys Rev Lett; 2001 Jul; 87(5):051101. PubMed ID: 11497756
    [TBL] [Abstract][Full Text] [Related]  

  • 12. The formation of massive star systems by accretion.
    Krumholz MR; Klein RI; McKee CF; Offner SS; Cunningham AJ
    Science; 2009 Feb; 323(5915):754-7. PubMed ID: 19150809
    [TBL] [Abstract][Full Text] [Related]  

  • 13. Foundations of Black Hole Accretion Disk Theory.
    Abramowicz MA; Fragile PC
    Living Rev Relativ; 2013; 16(1):1. PubMed ID: 28179840
    [TBL] [Abstract][Full Text] [Related]  

  • 14. Local model for angular-momentum transport in accretion disks driven by the magnetorotational instability.
    Pessah ME; Chan CK; Psaltis D
    Phys Rev Lett; 2006 Dec; 97(22):221103. PubMed ID: 17155789
    [TBL] [Abstract][Full Text] [Related]  

  • 15. Imprint of accretion disk-induced migration on gravitational waves from extreme mass ratio inspirals.
    Yunes N; Kocsis B; Loeb A; Haiman Z
    Phys Rev Lett; 2011 Oct; 107(17):171103. PubMed ID: 22107500
    [TBL] [Abstract][Full Text] [Related]  

  • 16. The rotating wind of the quasar PG 1700+518.
    Young S; Axon DJ; Robinson A; Hough JH; Smith JE
    Nature; 2007 Nov; 450(7166):74-6. PubMed ID: 17972879
    [TBL] [Abstract][Full Text] [Related]  

  • 17. Analog of astrophysical magnetorotational instability in a Couette-Taylor flow of polymer fluids.
    Boldyrev S; Huynh D; Pariev V
    Phys Rev E Stat Nonlin Soft Matter Phys; 2009 Dec; 80(6 Pt 2):066310. PubMed ID: 20365270
    [TBL] [Abstract][Full Text] [Related]  

  • 18. Angular momentum transport and particle acceleration during magnetorotational instability in a kinetic accretion disk.
    Hoshino M
    Phys Rev Lett; 2015 Feb; 114(6):061101. PubMed ID: 25723200
    [TBL] [Abstract][Full Text] [Related]  

  • 19. Magnetohydrodynamic stability of stochastically driven accretion flows.
    Nath SK; Mukhopadhyay B; Chattopadhyay AK
    Phys Rev E Stat Nonlin Soft Matter Phys; 2013 Jul; 88(1):013010. PubMed ID: 23944552
    [TBL] [Abstract][Full Text] [Related]  

  • 20. Identification of a non-axisymmetric mode in laboratory experiments searching for standard magnetorotational instability.
    Wang Y; Gilson EP; Ebrahimi F; Goodman J; Caspary KJ; Winarto HW; Ji H
    Nat Commun; 2022 Aug; 13(1):4679. PubMed ID: 35945242
    [TBL] [Abstract][Full Text] [Related]  

    [Next]    [New Search]
    of 5.