A change in the X-ray spectrum of Markarian 421

Astronomy and Astrophysics – Astronomy

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Bl Lacertae Objects, Spaceborne Astronomy, X Ray Sources, X Ray Spectra, Astronomical Models, Heao 1, Iue, Sas-3, Satellite Observation, Ultraviolet Spectra

Scientific paper

HEAO 1 A-2 experiment observations of the BL Lacertae object Mrk 421 in May 1978 show a marked spectral change from the OSO 8 observations of May 1977. The source was not detected above 10 keV in May 1978. The 2-10 keV spectrum could be well fitted by a power law with an energy slope of 2.2 to 4.2; thermal bremsstrahlung models with T less than 20 million are also acceptable. There was no indication of any low-energy turnover, so that the inferred column density is less than 7 x 10 to the 21st H atoms per sq cm. The total flux is consistent with an extrapolation of the UV data from IUE, but the slope is not consistent with the UV slope. Possible models for the origin of the spectral transition are discussed.

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