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H0323+022: Classification as a BL Lac and EXOSAT coordinated observations
Authors:H. Bradt  J. Baldwin  E. Feigelson  B. Geldzahler  G. Madejski  P. Massey  J. McClintock  I. McHardy  R. McMahan  T. Ohashi  R. Remillard  W. Romanishin  C. Salter  B. Schaefer  D. Schwartz  S. Tapia  J. Thorstensen  C. M. Urry  P. Wehinger  A. Wilson  S. Wyckoff
Affiliation:(1) 37-581 MIT, 02139 Cambridge, MA, USA;(2) CTIO, USA;(3) Penn State U., Pennsylvania, USA;(4) NRL, USA;(5) CFA, USA;(6) KPNO, USA;(7) MIT, USA;(8) U. Leicester, Leicester, USA;(9) Dartmouth College, Darmouth, UK;(10) Arizona State U, Arizona, USA;(11) NRAO, USA;(12) GSFC, USA;(13) CFA, USA;(14) U. Arizona, Arizona, USA;(15) U. Maryland, Maryland, USA
Abstract:The object H0323+022 (Doxsey et al. 1983) has been shown to be a BL Lac object by virtue of a diversity of observational characteristics at radio, optical, and x-ray wavelengths, in agreement with the conclusion of Margon and Jacoby (1984). Multi-frequency coordinated observations of this highly variable object with EXOSAT in September 1984 found it to be in a faint quiescent state (sim1/3; mgrJy at sim5 keV and V=16.55). Preliminary results from the latter observations are presented.
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