Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...232l..17m&link_type=abstract
Astrophysical Journal, Part 2 - Letters to the Editor, vol. 232, Aug. 15, 1979, p. L17-L19.
Astronomy and Astrophysics
Astronomy
37
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.
Boldt Elihu A.
Holt Stephen S.
Mushotzky Richard F.
Serlemitsos Peter J.
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