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14 ta ish

Ish: Instabilities in a nonstationary model of self-gravitating disks. III. The phenomenon of lopsidedness and a comparison of perturbation modes

  1. Physics of Gravitating Systems I

    A. M. Fridman, V. L. Polyachenko

    Kitob19847 iqtibos
    ABI

  2. Models of point mass clusters with quadratic gravitational potential.

    G. S. Bisnovatyj-Kogan, Ya. B. Zel’dovich

    Maqola19707 iqtibos
    ABI

  3. The Equilibria and Oscillations of a Family of Uniformly Rotating Stellar Disks

    Agris J. Kalnajs

    Maqola19725 iqtibos
    ABI

  4. Lopsided spiral galaxies

    Chanda J. Jog, Francoise Combes

    Maqola20094 iqtibos
    ABI

  5. Lopsided Spiral Galaxies and a Limit on the Galaxy Accretion Rate

    Dennis Zaritsky, Hans-Walter Rix

    Maqola19974 iqtibos
    ABI

  6. Lopsided spiral galaxies: evidence for gas accretion

    F. Bournaud, F. Combes, C. J. Jog +1

    Maqola20053 iqtibos
    ABI

  7. Lopsided galaxies

    J. E. Baldwin, D. Lynden–Bell, R. Sancisi

    Maqola19803 iqtibos
    ABI

  8. Production of Milky Way Structure by the Magellanic Clouds

    Martin D. Weinberg

    Maqola19952 iqtibos
    ABI

  9. Lopsided spiral galaxies

    A J. Jog, F. Combes

    Maqola20052 iqtibos
    ABI

  10. Sarlavhasiz

    Boshqa1 iqtibos
    ABI

  11. Sarlavhasiz

    Boshqa1 iqtibos
    ABI

  12. Sarlavhasiz

    Boshqa1 iqtibos
    ABI

  13. Sarlavhasiz

    Boshqa1 iqtibos
    ABI

  14. Sarlavhasiz

    Boshqa1 iqtibos
    ABI