Structure of the inner jet of OJ287 from VLBA data at 15 GHz in super-resolution mode
Tipo
Artigo
Data de publicação
2013
Periódico
Astrophysical Journal, Supplement Series
Citações (Scopus)
8
Autores
Tateyama C.E.
Orientador
Título da Revista
ISSN da Revista
Título de Volume
Membros da banca
Programa
Resumo
In this work we show the results obtained from the Very Long Baseline Array data at 15 GHz of OJ287 in super-resolution mode. The data showed a jet configuration in the form of a "fork" where superluminal components emerge via stationary components at the northwest and the southeast close to the core to form parallel trajectories along the southwest direction in the plane of sky. This agrees with a source structure of an extended, broad morphology of OJ287. © 2013. The American Astronomical Society. All rights reserved..