Infrared mapping of the M87 jet

Details Infrared mapping of the M87 jet Infrared mapping of the M87 jet

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...280..126k&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 280, May 1, 1984, p. 126-131.

Astronomy and Astrophysics

Astronomy

13

Elliptical Galaxies, Infrared Astronomy, Plasma Jets, Astronomical Photometry, Data Reduction

Scientific paper

Two-dimensional infrared images, in J, H, and K, of the M87 jet have been used to compute the fluxes of the brightest knots. The data in conjunction with existing radio and optical B band data are consistent with a power-law spectrum from the radio to the optical. Although the optical-UV and radio-IR spectral indices do indicate a break in spectral index somewhere in the optical region, the data together with those of de Vaucouleurs and Nieto are not consistent with a break between J and the optical B region.

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