Observations of the Andromeda Galaxy at 11-Centimeter Wavelength

Observations of the Andromeda galaxy (M31) at 2695 megahertz reveal more detail than do earlier measurements at lower frequency. The region is highly confused but there is apparently a more dense clustering of sources within the optical outline of the galaxy than without. One source (OA33) near M31...

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Published in:Science (American Association for the Advancement of Science) 1967-05, Vol.156 (3778), p.1087-1088
Main Authors: Cooley, R. C., Roberts, M. S., Swenson, G. W.
Format: Article
Language:English
Subjects:
Andromeda Galaxy
Antennas
Electromagnetic noise
Flux density
Light beams
Milky Way Galaxy
Spectral index
Wavelengths
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description Observations of the Andromeda galaxy (M31) at 2695 megahertz reveal more detail than do earlier measurements at lower frequency. The region is highly confused but there is apparently a more dense clustering of sources within the optical outline of the galaxy than without. One source (OA33) near M31 has an interesting, flat spectrum.
doi_str_mv 10.1126/science.156.3778.1087
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ispartof Science (American Association for the Advancement of Science), 1967-05, Vol.156 (3778), p.1087-1088
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source Science Magazine; JSTOR Archival Journals and Primary Sources Collection
subjects Andromeda Galaxy
Antennas
Electromagnetic noise
Flux density
Light beams
Milky Way Galaxy
Spectral index
Wavelengths
title Observations of the Andromeda Galaxy at 11-Centimeter Wavelength
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