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On the [OIII] emission of PG 1501+106

Published online by Cambridge University Press:  19 July 2016

G. M. Van Heerde
G. M. Van Heerde*
Affiliation:
Sterrewacht Leiden, Postbus, 9513 2300 RA LEIDEN

Abstract

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Narrow-band imaging of PG 1501+106 revealed no extra-nuclear [OIII] emission above a level of ∼ 20 μJy. The disagreement with the result of Boroson et. al., 1982 (who detected 40 μJy) can be explained by assuming a slight difference in angular size between the broad and narrow line emitting regions.

Type
III. Spectral Line Studies
Information
Symposium - International Astronomical Union , Volume 119: Quasars , 1986 , pp. 345 - 346
Copyright
Copyright © Reidel 1986 

References

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