The relationship of galaxy morphology to nuclear star formation in noninteracting spiral galaxies.
Three specific questions concerning the relationship between galaxian morphology and infrared properties were addressed for non-interacting galaxies: (1) Why are high infrared luminosity (L > 10¹⁰ L(⊙)) Sa galaxies scarce compared to Sb and Sc galaxies; (2) Is there a relationship between the bul...
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| Language: | en |
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The University of Arizona.
1989
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| Online Access: | http://hdl.handle.net/10150/184893 |