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The Velocity Field of NGC 1068

Published online by Cambridge University Press:  07 August 2017

N. Kaneko  and
T. Satoh
N. Kaneko
Affiliation:
Department of Physics, Hokkaido University, Sapporo 060, Japan
T. Satoh
Affiliation:
Kutchan Agricultural High School, Kutchan 044, Japan

Abstract

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Sixty spectra taken at 24 position angles of every 15° were measured for NGC 1068. The result reveals that a noncircular motion of about 50 km/s occurs within a spiral disk of 30″–40″ in radius.

Type
Part 6: Velocity Fields, Kinematics, NL Profiles
Information
Symposium - International Astronomical Union , Volume 134: Active Galactic Nuclei , 1989 , pp. 357 - 358
Copyright
Copyright © Kluwer 1989 

References

Ichikawa, S., Okamura, S., Kaneko, N., Nishimura, M., and Toyama, K. 1987, Publ. Astron. Soc. Japan 39, 411.Google Scholar
Kaneko, N., Morita, K., Fukui, Y., Sugitani, K., Iwata, T., Nakai, N., Kaifu, N., and Liszt, H. S. 1988, submitted to the Astrophys. J. Google Scholar
Nishimura, M., Kaneko, N., and Toyama, K. 1984, Astr. Astrophys. 130, 46.Google Scholar