The broad-band X-ray spectral variability of MRK 841

Details The broad-band X-ray spectral variability of MRK 841 The broad-band X-ray spectral variability of MRK 841

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.260..111g&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 260, no. 1, p. 111-120.

Astronomy and Astrophysics

Astronomy

24

Markarian Galaxies, Seyfert Galaxies, Variability, X Ray Spectra, Astronomical Spectroscopy, Emission Spectra, Exosat Satellite, Ginga Satellite, Spaceborne Astronomy, Spectral Line Width

Scientific paper

A detailed spectral analysis of five X-ray observations of Mrk 841 with the EXOSAT, Ginga, and ROSAT satellites is reported. Variability is apparent in both the soft (0.1-1.0 keV) and medium (1-20 keV) energy bands. Above, 1 keV, the spectra are adequately modeled by a power law with a strong emission line of equivalent width 450 eV. The large equivalent width of the emission line indicates a strongly enhanced reflection component of the source compared with other Seyferts observed with Ginga. The implications of the results of the analysis for physical models of the emission regions in this and other X-ray bright Seyferts are briefly examined.

Affiliated with

Also associated with

No associations

Rating

The broad-band X-ray spectral variability of MRK 841 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The broad-band X-ray spectral variability of MRK 841, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The broad-band X-ray spectral variability of MRK 841 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1262993