X ray spectra of bright BL Lacertae objects observed with ROSAT

Details X ray spectra of bright BL Lacertae objects observed with ROSAT X ray spectra of bright BL Lacertae objects observed with ROSAT

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992xrea.conf..202f&link_type=abstract

In its X Ray Emission from Active Galactic Nuclei and the Cosmic X Ray Background p 202-205 (SEE N93-17094 05-90)

Astronomy and Astrophysics

Astronomy

6

Absorption Spectra, Bl Lacertae Objects, Rosat Mission, X Ray Spectra, Brightness Distribution, Indexes (Ratios), Sky Surveys (Astronomy), Spectral Signatures, Spectrum Analysis, X Ray Astronomy

Scientific paper

The soft X-ray data of 10 bright BL Lacertae objects observed during the Rosat All Sky Survey (RASS) were analyzed in order to compare their spectral characteristics. The spectra are well described by simple power law models. No indications for intrinsic absorption were found. The steep spectral indices of all spectra are very similar. In the spectra of three BL Lacertae absorption features below 1 keV, although statistically insignificant, cannot be excluded.

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