The X-ray emission of 3C273

Details The X-ray emission of 3C273 The X-ray emission of 3C273

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.244..310t&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 244, May 15, 1990, p. 310-321.

Astronomy and Astrophysics

Astronomy

94

Emission Spectra, Quasars, X Ray Sources, Accretion Disks, Exosat Satellite, Iron, Line Spectra, Red Shift

Scientific paper

Exosat and Ginga observations of the X-ray emission of 3C273 in the 0.2-35 keV band are reported for the period from December, 1983 to December, 1988. No standard models adequately describe the behavior revealed by the Exosat and Ginga data. The characteristics of the observations are described. Variations with time in the spectral index are not correlated with the overall X-ray flux level. The observations suggest that the iron line is independent of variations in the 2-10 keV flux.

Affiliated with

Also associated with

No associations

Rating

The X-ray emission of 3C273 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 X-ray emission of 3C273, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The X-ray emission of 3C273 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-783106