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1411+442: Optical Imaging of a BAL QSO

Published online by Cambridge University Press:  04 August 2017

J.B. Hutchings
J.B. Hutchings*
Affiliation:
Dominion Asyrophysical Observatory, 5071 W. Saanich Rd., Victoria, BC, Canada

Abstract

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Results are presented of optical imaging of the low redshift BAL QSO 1411+442, in four colours. The host galaxy is revealed as an inclined spiral galaxy with a long arm which may be a tidal tail. There also appears to be connecting luminosity to two nearby objects. There is a straight blue feature emerging from the nucleus and Ha emission from an oppositely directed filament. [O III] appears to be enhanced in some outer regions. While the host galaxy is more exotic than usual for QSOs, it is not obvious how these properties are connected with the BAL phenomenon.

Type
VI. Environmental Aspects of Nuclear Activity
Information
Symposium - International Astronomical Union , Volume 121: Observational Evidences of Activity of Galaxies , 1987 , pp. 395 - 397
Copyright
Copyright © Reidel 1987 

References

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