The spectral energy distribution of NGC 1275

Details The spectral energy distribution of NGC 1275 The spectral energy distribution of NGC 1275

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975stin...7526939s&link_type=abstract

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Astronomy and Astrophysics

Astronomy

Interstellar Gas, Radio Galaxies, Spectral Energy Distribution, Constellations, Cosmic Gases, Nonthermal Radiation, Radio Astronomy, Spectral Emission, Stellar Radiation

Scientific paper

An analysis of absolute spectral energy distributions of interstellar gas for a galaxy (NGC 1275) is presented. Infrared spectra data shows heavy reddening. It is proposed that the interstellar gas may be ionized by shock waves or by nonthermal or stellar radiation. It is suggested, that high velocity, emission-line knots are H2 regions in a Perseus cluster galaxy or intergalactic gas cloud seen in projection against NGC 1275.

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