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Three-Dimensional Fabry-Perot Imaging Spectroscopy of the Crab Nebula

Published online by Cambridge University Press:  12 April 2016

Stephen S. Lawrence ,
Gordon M. MacAlpine ,
Alan Uomoto ,
Richard Gelderman ,
Bruce E. Woodgate  and
Larry W. Brown
Stephen S. Lawrence
Affiliation:
Dept. of Astronomy, University of Michigan, Ann Arbor, MI 48109, U.S.A.
Gordon M. MacAlpine
Affiliation:
Dept. of Astronomy, University of Michigan, Ann Arbor, MI 48109, U.S.A.
Alan Uomoto
Affiliation:
Dept. of Physics and Astronomy, The Johns Hopkins University, Baltimore, MD 21218, U.S.A.
Richard Gelderman
Affiliation:
NASA Goddard Space Flight Center, Greenbelt, MD 20771, U.S.A.
Bruce E. Woodgate
Affiliation:
NASA Goddard Space Flight Center, Greenbelt, MD 20771, U.S.A.
Larry W. Brown
Affiliation:
NASA Goddard Space Flight Center, Greenbelt, MD 20771, U.S.A.

Abstract

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A three-dimensional model of the [O III] λ5007 line-emitting gas in the Crab Nebula has been developed from imaging spectroscopy taken with the Goddard Fabry-Perot Imager mounted on the McGraw-Hill 1.3m telescope of Michigan-Dartmouth-MIT Observatory. Several interesting morphological features revealed in three-dimensional isophotal displays are discussed.

Type
2. The Fabry-Perot Spectrometer and its Applications
Information
International Astronomical Union Colloquium , Volume 149: Tridimensional Optical Spectroscopic Methods in Astrophysics , 1995 , pp. 165 - 166
Copyright
Copyright © Astronomical Society of the Pacific 1995

References

Gelderman, R., Woodgate, B., and Brown, L. 1994, these proceedingsGoogle Scholar
Lawrence, S.S., MacAlpine, G.M., Uomoto, A., Woodgate, B.E., Brown, L.W., and Oliversen, R.J. 1994, in preparationGoogle Scholar
MacAlpine, G.M., McGaugh, S.S., Mazzarella, J.M., and Uomoto, A. 1989, ApJ, 342, 364 CrossRefGoogle Scholar
Uomoto, A. and MacAlpine, G.M. 1987, AJ, 93, 1511 CrossRefGoogle Scholar