Weak Radio Galaxies: Narrow-Band Optical Imaging
1996 ◽
Vol 175
◽
pp. 236-237
Keyword(s):
Previous studies show that: a) radio galaxies and radio-loud quasars have emission-line gas (ELG) which is extended on scales of tenths of kiloparsecs; b) there is convincing evidence that the kinematics and excitation of the very extended emission-line gas is governed by its interaction with the outflowing radio plasma; c) the evidence for an interaction is weaker in some radio galaxies. It is argued that the ionization of the ELG may be predominantly produced by the nuclear ultraviolet continuum and the kinematics of the gas due to the gravitational potential of the host galaxy, but it is not yet known whether there is a physical relationship between the ELG and the extended radio jets.
Keyword(s):
1996 ◽
Vol 175
◽
pp. 227-229
Keyword(s):
Keyword(s):
2020 ◽
Vol 494
(2)
◽
pp. 2053-2067
Keyword(s):
1996 ◽
Vol 175
◽
pp. 471-472
Keyword(s):
2020 ◽
Vol 15
(S359)
◽
pp. 307-311
Keyword(s):
1997 ◽
Vol 159
◽
pp. 392-393
Keyword(s):
2001 ◽
Vol 205
◽
pp. 194-195
Keyword(s):
2004 ◽
Vol 351
(3)
◽
pp. 997-1014
◽
Keyword(s):