Author： Arribas S. Mediavilla E. Garcia-Lorenzo B. Del Burgo C.
Publisher： Springer Publishing Company
ISSN： 0004-640X
Source： Astrophysics and Space Science, Vol.248, Iss.1-2, 1997-01, pp. : 159-166
Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.
Abstract
From 2-D spectroscopy of the [O III] 4959,5007 and [S III] 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.
Related content
By Mediavilla E. Arribas S. Garcia-Lorenzo B. Del Burgo C.
Astrophysics and Space Science, Vol. 248, Iss. 1-2, 1997-01 ,pp. :
Access to resources
Recommend
Ultraviolet Lines and Gas Composition in NGC 1068
By Netzer H.
Astrophysics and Space Science, Vol. 248, Iss. 1-2, 1997-01 ,pp. :
By Schartmann M. Burkert A. Krause M. Camenzind M. Meisenheimer K. Davies R. I.
Monthly Notices of the Royal Astronomical Society, Vol. 403, Iss. 4, 2010-04 ,pp. :
Vertical Velocity Dispersion of the Ionized Gas In NGC 3938
Astrophysics and Space Science, Vol. 276, Iss. 2-4, 2001-01 ,pp. :