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Two X-ray-selected BL Lacertae objects observed with the HEAO 1 scanning modulation collimatorTwo 16th magnitude BL Lac objects, H1101 - 232 and H1426 + 428, have been discovered. Each is a persistent and relatively bright X-ray source. A 2.7 percent linear polarization is measured in the optical emission or H101 - 232. The X-ray identification of H1426 + 428 is confirmed in an Exosat observation. The X-ray spectrum is well-modeled by a power law with an energy index of 1.19. Both BL Lac objects exhibit high f(x)/f(opt) ratios and they show a distinct resemblance to other X-ray selected BL Lac objects. The host galaxies are about 18th mag with angular diameters of about 20 arcsec and each may be the dominant member of a cluster of galaxies. Additional wide-slit spectroscopy reveals faint absorption features with redshifts of 0.129 for H1426 + 428 and 0.186 for H1101 - 232. The implied X-ray and optical luminosities exceed 10 to the 45th ergs/s for both BL Lac nuclei, assuming isotropic emission.
Document ID
19900023712
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Remillard, R. A.
(MIT Cambridge, MA, United States)
Tuohy, I. R.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Brissenden, R. J. V.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Buckley, D. A. H.
(Mount Stromlo and Siding Spring Observatories Canberra, Australia)
Schwartz, D. A.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Date Acquired
August 14, 2013
Publication Date
October 1, 1989
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 345
ISSN: 0004-637X
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0004-637X
Accession Number
90A10767
Funding Number(s)
CONTRACT_GRANT: NSF AST-83-51447
CONTRACT_GRANT: NSF INT-82-11357
CONTRACT_GRANT: NAG8-493
CONTRACT_GRANT: NAS8-27972
CONTRACT_GRANT: NAS8-30453
CONTRACT_GRANT: NSF AST-86-12572
CONTRACT_GRANT: NSF AST-84-14591
Distribution Limits
Public
Copyright
Other

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