X-ray emission from the jet of M87.

Details X-ray emission from the jet of M87. X-ray emission from the jet of M87.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996rftu.proc..489n&link_type=abstract

International Conference on X-ray Astronomy and Astrophysics: Röntgenstrahlung from the Universe, p. 489 - 490

Astronomy and Astrophysics

Astrophysics

Elliptical Galaxies: Jets, Elliptical Galaxies: X Rays

Scientific paper

The jet of the giant elliptical galaxy M87 is one of the few objects of its kind allowing detailed morphological studies from radio wavelengths up to the X-ray regime. While the synchrotron nature of its radio to optical continuum is established, it is still unclear what causes the X-ray emission. The authors discuss this question by comparing ROSAT-HRI data with the radio to optical synchrotron emission of the jet.

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