Hostname: page-component-8448b6f56d-cfpbc Total loading time: 0 Render date: 2024-04-24T03:52:59.584Z Has data issue: false hasContentIssue false
  • English
  • Français

Nuclear Activity in the Seyfert Galaxy NGC 1365

Published online by Cambridge University Press:  19 July 2016

M. Hjelm ,
P.O. Lindblad  and
S. Jörsäter
M. Hjelm
Affiliation:
Stockholm Observatory, 133 36 Saltsjöbaden, Sweden
P.O. Lindblad
Affiliation:
Stockholm Observatory, 133 36 Saltsjöbaden, Sweden
S. Jörsäter
Affiliation:
Stockholm Observatory, 133 36 Saltsjöbaden, Sweden

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

NGC 1365 is a barred Seyfert 1.5 galaxy. Fig 1a is a contour plot of an [OIII]λ5007 image (Jörsäter & Lindblad 1989), showing a plume-like structure pointing towards SE in the direction of the minor axis of the galaxy, which also is the direction of the steepest velocity gradient in [OIII]λ5007. The plume is roughly aligned with a radio feature in the 6 and 20 cm continuum (see Sandqvist et al., this volume). The [OIII]-emission on the NW side is weaker. This plume-like structure is not seen in Hα.

Type
Poster Contributions: Line Studies
Information
Symposium - International Astronomical Union , Volume 159: Multi-Wavelength Continuum Emission of AGN , 1994 , pp. 448
Copyright
Copyright © Kluwer 1994 

References

Hjelm, M., Lindblad, P.O. and Jörsäter, S., 1994, in prep.Google Scholar
Jörsäter, S. and Lindblad, P.O., 1989, ESO Workshop on Extra Nuclear Activity, p 39.Google Scholar