Angular Momentum and Mass Redistribution Induced by Gravitationally (Jeans-) Unstable Spiral Density Waves in Disks of Flat Galaxies

Research output: Non-textual form › Digital or Visual Products

Abstract

Disks of galaxies are efficient at mass and angular momentum transfer on the timescale of an order of 2-3 rotational periods.

Original language	English
State	Published - 1 Oct 2008

@misc{3b723112c0fc4b15a3adf4e401e5388b,

title = "Angular Momentum and Mass Redistribution Induced by Gravitationally (Jeans-) Unstable Spiral Density Waves in Disks of Flat Galaxies",

abstract = "Disks of galaxies are efficient at mass and angular momentum transfer on the timescale of an order of 2-3 rotational periods.",

author = "E. Liverts and E. Griv and M. Gedalin and M. Mond",

year = "2008",

month = oct,

day = "1",

language = "English",

volume = "396",

}

TY - ADVS

T1 - Angular Momentum and Mass Redistribution Induced by Gravitationally (Jeans-) Unstable Spiral Density Waves in Disks of Flat Galaxies

AU - Liverts, E.

AU - Griv, E.

AU - Gedalin, M.

AU - Mond, M.

PY - 2008/10/1

Y1 - 2008/10/1

N2 - Disks of galaxies are efficient at mass and angular momentum transfer on the timescale of an order of 2-3 rotational periods.

AB - Disks of galaxies are efficient at mass and angular momentum transfer on the timescale of an order of 2-3 rotational periods.

M3 - Digital or Visual Products

VL - 396

ER -