Published November 1976 | Version v1
Journal article

The possible origin of the spiral-arm instability

Creators

  • 1. Michigan Univ., Ann Arbor (USA). Dept. of Astronomy

Description

Physical arguments suggest the spiral arms may be manifestations of the galaxy not being in dynamical equilibrium - in the sense that the kinetic energy of its stars and gas is less relative to its binding energy than that dictated by the virial theorem. Without constant cooling of the galactic disk (i.e., a progressive increase in the binding energy of the galaxy) such a departure from dynamical equilibrium would be corrected and the spiral arms destroyed in about 109 yr due to an increase in the velocity dispersion of the stars in the disk resulting from their interacting with the spiral arms. The rate of cooling required to maintain the spiral arms, may be proved by mass loss from stars in the disk population. The cooling arises from the average scale-heights and velocities of these stars being larger than that of the gas in the disk, so that there is a net loss of kinetic energy and an increase in the binding energy of the galaxy due to the ejected gas settling down to a lower terminal velocity and scale-height in the galactic disk. (Auth.)

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysics and Space Science
Journal Volume
45
Journal Issue
1
Series
Astrophys. Space Sci.
Journal Page Range
243-248
ISSN
0004-640X

INIS

Country of Publication
Netherlands
Country of Input or Organization
Netherlands
INIS RN
8308563
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ANGULAR VELOCITY; BINDING ENERGY; BOUNDARY CONDITIONS; COOLING; COSMIC GASES; EQUILIBRIUM; GALAXIES; INSTABILITY; INTERSTELLAR SPACE; KINETIC ENERGY; ORBITS; POTENTIAL ENERGY; ROTATION; VIRIAL THEOREM
Descriptors DEC
ENERGY; FLUIDS; GASES; SPACE; VELOCITY

Optional Information

Notes
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