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Emission Lines in Active Galaxies: Outlook for the Future

Published online by Cambridge University Press:  12 April 2016

Bradely M. Peterson
Bradely M. Peterson*
Affiliation:
Department of Astronomy, The Ohio State University, 174 West 18th Avenue, Columbus, OH 43210, USA

Abstract

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I briefly outline some of the unanswered questions that have emerged as recurring themes at this conference and offer some speculation about how these will be addressed with new techniques and facilities of the future.

Type
XL. Summary
Information
International Astronomical Union Colloquium , Volume 159: Emission Lines in Active Galaxies: New Methods and Techniques , 1997 , pp. 489 - 497
Copyright
Copyright © Astronomical Society of the Pacific 1997

References

Alloin, D, Clavel, J., Peterson, B.M., Reichert, G.A., & Stirpe, G.M. 1994, in Frontiers of Space and Ground-Based Astronomy, ed. Wamsteker, W., Longair, M.S., & Kondo, Y., Kluwer Academic Pub., p. 325.CrossRefGoogle Scholar
Blandford, R.D. 1992, in Relationships Between Active Galactic Nuclei and Star-burst Galaxies, ed. Filippenko, A.V., Astronomical Society of the Pacific Conference Series, Vol. 31, p. 29.Google Scholar
Done, C., & Krolik, J.H. 1996, ApJ, 463, 144.CrossRefGoogle Scholar
Douglas, K.N., Robinson, I., Schild, A., Schucking, E.L., Wheeler, J.A., & Woolf, N.J., editors. 1969, Quasars and High-Energy Astronomy (Gordon and Breach: New York).Google Scholar
Ford, H.C., Harms, R.J., Tsvetanov, Z.I., Hartig, G.F., Dressel, L.L., Kriss, G.A., Bohlin, R.C., Davidsen, A.F., Margon, B., & Kochhar, A.K. 1994, ApJ, 435, L27.Google Scholar
Harms, R.J., Ford, H.C., Tsvetanov, Z.L., Hartig, G.F., Dressel, L.L., Kriss, G.A., Bohlin, R., Davidsen, A.F., Margon, B., & Kochhar, A.K. 1994, ApJ, 435, L31.CrossRefGoogle Scholar
Korista, K.T., et al. 1995, ApJS, 97, 285.Google Scholar
Kormendy, J., & Richstone, D. 1995, ARAA, 33, 581.CrossRefGoogle Scholar
Miyoshi, M., Moran, J., Herrnstein, J., Greenhill, L., Nakai, N., Diamond, P., & Inoue, M. 1995, Nature, 373, 127.CrossRefGoogle Scholar
Osterbrock, D.E., Koski, A., & Phillips, M.M. 1976, ApJ, 206, 298.Google Scholar
Stengler-Larrea, E.A., et al. ApJ, 444, 64.Google Scholar
Tanaka, Y., et al. 1995, Nature, 375, 659.CrossRefGoogle Scholar
Wanders, I., Goad, M.R., Korista, K.T., Peterson, B.M., Horne, K., Ferland, G.J., Koratkar, A.P., Pogge, R.W., & Shields, J.C. 1995, ApJ, 453, L87.CrossRefGoogle Scholar
Warren, S.J., Hewett, P.C., & Osmer, P.S. 1994, ApJ, 421, 412.Google Scholar
Yee, H.C.K., & Oke, J.B. 1981, ApJ, 248, 472.CrossRefGoogle Scholar
Zanstra, H. 1931, Pub. Dominion Astrophys. Obs., 4, 209.Google Scholar