In:
International Astronomical Union Colloquium, Cambridge University Press (CUP), Vol. 159 ( 1997), p. 215-216
Abstract:
A hydromagnetic wind model from a dusty molecular disk (Emmering, Blandford, & Shlosman 1992) was applied to the BLR in NGC 5548 and produced synthetic C IV line profiles as a function of time. The model C IV profiles are compared to data from the 1993 IUE/HST campaign and properties of the the BLR of NGC 5548 are inferred.
Type of Medium:
Online Resource
ISSN:
0252-9211
DOI:
10.1017/S0252921100040082
Language:
English
Publisher:
Cambridge University Press (CUP)
Publication Date:
1997
detail.hit.zdb_id:
1099007-0