NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Collections About News Help Login
Back to Results
A wind-type model for the generation of astrophysical jetsWind-type solutions for the generation of astrophysical jets from active galactic nuclei and stellar sources, such as those associated with SS 433 and protostellar objects, are discussed. Acceleration, collimation, and morphology are consistently interpreted in terms of a flow starting from the galactic or stellar core inside the 'throat' of a thick accretion disk.
Document ID
19840043190
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/184197
Authors
Ferrari, A. (Harvard-Smithsonian Center for Astrophysics, Cambridge, MA; Torino, Universita Turin, Italy)
Habbal, S. R. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Rosner, R. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Tsinganos, K. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Date Acquired
August 12, 2013
Publication Date
February 15, 1984
Publication Information
Publication: Astrophysical Journal, Part 2 - Letters to the Editor
Volume: 277
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
84A25977
Funding Number(s)
CONTRACT_GRANT: NAGW-249
CONTRACT_GRANT: NSF AST-83-03522
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.

Related Records

There are no records associated with this record.
No Preview Available