The spectral energy distribution of NGC 1275
Technical Report
·
OSTI ID:7350896
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. (Author) (GRA)
- Research Organization:
- Hale Observatories, Pasadena, Calif. (USA)
- OSTI ID:
- 7350896
- Report Number(s):
- N-75-26939/9ST; NASA-CR-143039
- Country of Publication:
- United States
- Language:
- English
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