On the Distribution of Matter Within Highly Flattened Galaxies.
From MaRDI portal
Publication:3846319
DOI10.1086/147653zbMath0109.23403OpenAlexW2056918564WikidataQ68201270 ScholiaQ68201270MaRDI QIDQ3846319
Publication date: 1963
Published in: The Astrophysical Journal (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1086/147653
Related Items
Simple distribution functions for stellar systems ⋮ Galactic dynamics in general relativity: the role of gravitomagnetism ⋮ Exact relativistic models of conformastatic charged dust thick disks ⋮ Spiral galaxy rotation curves determined from Carmelian general relativity ⋮ Orbital perturbations due to massive rings ⋮ General magnetized Weyl solutions: disks and motion of charged particles ⋮ Exact relativistic models of perfect fluid disks in a magnetic field ⋮ EXACT RELATIVISTIC MODELS OF THIN DISKS AROUND STATIC BLACK HOLES IN A MAGNETIC FIELD ⋮ Computer simulation of three-dimensional stellar systems in cylindrical coordinates ⋮ Models of spherical shells as sources of Majumdar-Papapetrou type spacetimes ⋮ RELATIVISTIC RING MODELS ⋮ Probing Yukawian gravitational potential by numerical simulations. I: Changing \(N\)-body codes ⋮ New formulation of the theory of finite galactic disks ⋮ On a general fluid dynamical theory of discrete unstable spiral modes in disk-shaped galaxies ⋮ General relativistic razor-thin disks with magnetically polarized matter ⋮ A solution for galactic disks with Yukawian gravitational potential ⋮ A gaseous shock wave theory of the galactic spiral structure
