Ionized Gas Velocity Field in Central Region of NGC 1068 Inferred from the [O III] λλ 4959,5007 and [S III] λ 9069 Lines

Bibcode
1997Ap&SS.248..159A
DOI
10.1023/A:1000521410414
Arribas, S.; Mediavilla, E.; Garcia-Lorenzo, B.; Del Burgo, C.
Bibliographical reference

Astrophysics and Space Science, Volume 248, Issue 1-2, pp. 159-166

Advertised on:
2
1997
Journal
Astrophysics and Space Science
Number of authors
4
IAC number of authors
4
Citations
2
Refereed citations
2
Description
From 2-D spectroscopy of the [O III] λλ 4959,5007 and [S III] λ 9069 lines we have studied the ionized gas-velocity field in the central regions of NGC 1068. The existence of a strong bipolar outflow of ionized gas is confirmed. The origin of this outflow, which is probably related to the active nucleus, is about 1.4″ NE of the optical nucleus; therefore, this region is a candidate to host the hidden nucleus of NGC 1068.
Type
Refereed

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