IRAS observations of NGC 1052
Journal Article
·
· Publ. Astron. Soc. Pac.; (United States)
The galaxy NGC 1052 has been observed with the IRAS satellite. The infrared emission at 100 microns is substantially larger than a smooth extrapolation of the radio data. Because of the large diaphragm size of IRAS, it is impossible to decide uniquely if the infrared radiation represents a self-absorbed nonthermal spectrum or thermal reradiation by heated dust. 23 references.
- Research Organization:
- California Institute of Technology (CalTech), Pasadena, CA (United States)
- OSTI ID:
- 5826907
- Journal Information:
- Publ. Astron. Soc. Pac.; (United States), Vol. 96
- Country of Publication:
- United States
- Language:
- English
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