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Filamentary Nebulosity Surrounding M87

Published online by Cambridge University Press:  04 August 2017

S. van den Bergh  and
C. J. Pritchet
S. van den Bergh
Affiliation:
Dominion Astrophysical Observatory
C. J. Pritchet
Affiliation:
University of Victoria

Extract

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Recently we have obtained both Hα + [NII] and broad-band red exposures of a number of galaxies with an RCA 320 × 512 CCD at the prime-focus of the 3.6 m CFH Telescope. Figure 1 shows the difference between Hα and red exposures (each with a total integration time of 60 min) of M87 = NGC4486.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 117: Dark Matter in the Universe , 1987 , pp. 216 - 217
Copyright
Copyright © Reidel 1987 

References

Arp, H.C. 1967. Ap. Letters 1, 1.Google Scholar
De Young, D.S., Condon, J.J. and Butcher, H. 1980. Ap. J. 242, 511.CrossRefGoogle Scholar
Ford, H.C., and Butcher, H. 1979. Ap. J. Suppl. 41, 147.CrossRefGoogle Scholar
Lynds, R. 1970. Ap. J. (Letters) 159, L151.Google Scholar