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Author > Byrd, G. G. 
Author > Miller, R. H. 
Author > Smith, B. F. 

NASA Center > Ames Research Center 

Publication Year > 1981-1990 > 1984 

Subject > A-C > Astrophysics 

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Item/Media Type > Journal Article 


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Title: Gravitational spurs and resonances - Effects of small mass disturbers in spiral galaxy disks
Author(s): Byrd, G. G.; Smith, B. F.; Miller, R. H.
Abstract: In the present simulations of a disturber in a complete stellar disk without the restrictive assumption, the disturber parameters of the NGC 206 cloud in M 31 were assumed as a realistic example. The resulting spur around the disturber was comparable in shape, size, and strength to Julian and Toomre's (1966) results. In addition, a complicated evolving pattern of strong density peaks appeared well inside and outside the disturber's orbit. Simulation with a ten-times-more-massive disturber showed a more clearly defined version of the same initial pattern, two spiral arms of density peaks rotating with the disturber in the stronger arm. The orbital radii of the density peaks correspond to those of epicyclic resonances with the orbiting disturber potential.
NASA Center: Ames Research Center
Publication Date: Nov 1, 1984
Document Source: Other Sources
No Digital Version Available: Go to Tips On Ordering
Document ID: 19850036032
Accession ID: 85A18183
Publication Information: Astrophysical Journal, Part 1, 286, 62-67, ISSN 0004-637X, Number of Pages = 6
Related Information: Research supported by the University of Alabama and American Astronomical Society
Keywords: ASTRONOMICAL MODELS; GALACTIC STRUCTURE; GRAVITATIONAL EFFECTS; GRAVITATIONAL FIELDS; MASS DISTRIBUTION; SPIRAL GALAXIES; ANDROMEDA GALAXY; COSMIC GASES; GALACTIC EVOLUTION; MOLECULAR CLOUDS; ORBITAL ELEMENTS; RADII;
Notes: Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 286, Nov. 1, 1984, p. 62-67. Research supported by the University of Alabama and American Astronomical Society.
Accessibility: Unclassified; Copyright; Unlimited; Publicly available;
Updated/Added to NTRS: 2004-11-03

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