Abstract
The emission components of spiral galaxies between 12 microns and 90 cm are identified. Additionally, an attempt to understand the relationships between them was made. The specific goal was to gain some understanding on the nature of the radio-infrared correlation. The results are summarized.
Cite
CITATION STYLE
APA
Frohlich, E. D., Ré, R. N., & Navar, L. G. (1999). Annual Progress Report. Hypertension, 33(1), 1–6. https://doi.org/10.1161/01.hyp.33.1.1
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