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Extended Line Emitting Regions in the Seyfert Galaxy NGC 2992

Published online by Cambridge University Press:  04 August 2017

L. Colina ,
K.J. Fricke ,
W. Kollatschny  and
M.A.C. Perryman
L. Colina
Affiliation:
Universitäts-Sternwarte Göttingen, West Germany
K.J. Fricke
Affiliation:
Universitäts-Sternwarte Göttingen, West Germany
W. Kollatschny
Affiliation:
Universitäts-Sternwarte Göttingen, West Germany
M.A.C. Perryman
Affiliation:
ESA-ESTEC. Space Science Department, Astrophysics Division, Noordwijk, Netherlands

Extract

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NGC 2992 is a nearby Seyfert galaxy (z=0.008, 1″=150 pc, for HO=75 km s−1 Mpc−1) seen almost edge-on (i=70°). A dust lane crossing the galaxy has been detected (Burbidge et al. 1972, see also Fig. 1) and the presence of two extended radio-emitting regions at position angles P.A. 130° and P.A. 160° has been reported (Ulvestad and Wilson, 1984).

Type
III. Seyfert Galaxies
Information
Symposium - International Astronomical Union , Volume 121: Observational Evidences of Activity of Galaxies , 1987 , pp. 131 - 133
Copyright
Copyright © Reidel 1987 

References

Literature

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