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First Results with HIFI: Studies of Extended Anomalous Emission Regions with an Imaging Fabry-Perot

Published online by Cambridge University Press:  07 August 2017

R. Brent Tully ,
Jonathan Bland  and
Gerald Cecil
R. Brent Tully
Affiliation:
Institute for Astronomy, University of Hawaii
Jonathan Bland
Affiliation:
University of Hawaii and Rice University
Gerald Cecil
Affiliation:
Institute for Advanced Studies

Abstract

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The new imaging Fabry-Perot interferometer at the University of Hawaii is especially suited for studying extended emission regions in the vicinity of active nuclei. Dramatic results have been obtained for the objects observed so far: M51, M82, NGC 1068, NGC 4151, and NGC 4258.

Type
Part 6: Velocity Fields, Kinematics, NL Profiles
Information
Symposium - International Astronomical Union , Volume 134: Active Galactic Nuclei , 1989 , pp. 337 - 342
Copyright
Copyright © Kluwer 1989 

References

Axon, D. J., and Taylor, K. 1978, Nature, 274, 37.Google Scholar
Bland, J., and Tully, R. B. 1988a, Nature, 334, 43.Google Scholar
Bland, J., and Tully, R. B. 1988b, A. J., (submitted).Google Scholar
Boulesteix, J., Georgelin, Y. P., Marcelin, M., and Monnet, G. 1983, SPIE Conf. Inst. Astron. V, 445, 37.Google Scholar
Cecil, G. N. 1988, Ap. J., 329, 38.CrossRefGoogle Scholar
Chevalier, R.A. and Clegg, A.W., Nature, 317, 44.Google Scholar
Crane, P. C., van der Hulst, J. M., Ford, H. C., Lawrie, D. G., and Jacoby, G. H. 1987, Bull. A. A. S., 19, 681.Google Scholar
Courtès, G. 1964, A. J., 69, 325.CrossRefGoogle Scholar
Courtès, G., and Cruvellier, P. 1961, Comtes Rendus Acad. Sci. Paris, 253, 218.Google Scholar
de Vaucouleurs, G., and Pence, W. D. 1980, Ap. J., 242, 18.Google Scholar
Elvius, A. 1963, Lowell Obs. Bull., 5, 281.Google Scholar
Ford, H. C., Crane, P. C., Jacoby, G. H., Lawrie, D. G., and van der Hulst, J. M. 1985, Ap.J., 293, 132.Google Scholar
Hicks, T. R., Reay, N. K., and Atherton, P. D. 1984, J. Phys. E., 17, 49.Google Scholar
Kronberg, P. P., and Sramek, R. A. 1985, Science, 227, 28.CrossRefGoogle Scholar
Lynds, C. R., and Sandage, A. 1963, Ap. J., 137, 1005.Google Scholar
Sandage, A., and Miller, W. C. 1964, Science, 144, 405.Google Scholar
Solinger, A. B. 1969, Ap. J., 155, 403.CrossRefGoogle Scholar
Taylor, K., and Atherton, P. D. 1980, M. N. R. A. S., 191, 675.Google Scholar
Tully, R. B. 1974, Ap. J. Suppl., 27, 415.Google Scholar
van der Kruit, P. C., Oort, J. H., and Mathewson, D. S. 1972, Astr. Ap., 21, 169.Google Scholar
Watson, M. G., Stanger, V., and Griffiths, R. E. 1984, Ap. J., 286, 144.Google Scholar
Williams, T. B., Caldwell, N., and Schommer, R. A. 1984, Ap. J., 281, 579.Google Scholar