NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Collections About News Help Login
Back to Results
The evolution of protoplanetary disksAccretion disks evolve by transferring angular momentum outwards, which allows mass to flow inwards onto the central object. The radial structure and time-dependent behavior of low-mass, Keplerian, viscous disks is analyzed. Potential mechanisms for the angular momentum transport in disks are reviewed. An evolutionary model of a low mass disk around a pulsar is presented.
Document ID
19930052444
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Ruden, Steven P. (California Univ. Irvine, United States)
Date Acquired
August 16, 2013
Publication Date
January 1, 1993
Publication Information
Publication: In: Planets around pulsars; Proceedings of the Conference, California Inst. of Technology, Pasadena, Apr. 30-May 1, 1992 (A93-36426 14-90)
Publisher: Astronomical Society of the Pacific
Subject Category
Astrophysics
Accession Number
93A36441
Funding Number(s)
CONTRACT_GRANT: NAGW-2260
CONTRACT_GRANT: NSF AST-91-57420
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.

Related Records

IDRelationTitle19930052429Collected WorksPlanets around pulsars; Proceedings of the Conference, California Inst. of Technology, Pasadena, Apr. 30-May 1, 1992
No Preview Available