Are BL Lac objects too large to be gravitationally lensed?

Gear, Walter Kieran 1991. Are BL Lac objects too large to be gravitationally lensed? Nature 349 (6311) , pp. 676-678. 10.1038/349676a0

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Abstract

BL LACERTAEobjects are extragalactic sources, generally of low redshift, with highly variable, strongly polarized continuum emission ranging from radio wavelengths to X-rays, but with little or no evidence of line emission. It has been suggested1that BL Lacs are in fact more distant radio-loud, optically violently variable (OVV) quasars whose continuum is enhanced, relative to the line emission, by gravitational lensing caused by a star in an intervening galaxy. I argue here, however, that the spectral similarity of BL Lacs and OWs over a wide wavelength range can be explained by gravitational lensing only if the continuum-emitting region is small, a requirement that is contradicted by independent observations.

Item Type:	Article
Date Type:	Publication
Status:	Published
Schools:	Physics and Astronomy
Subjects:	Q Science > QB Astronomy
Publisher:	Macmillan Publishers Ltd.
ISSN:	0028-0836
Last Modified:	04 Jun 2017 04:17
URI:	http://orca.cf.ac.uk/id/eprint/36076

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