MASSIVE STAR FORMATION IN TWO SPIRAL GALAXIES: NGC 3938 AND NGC 3184; MULTIWAVELENGTH ANALYSIS
The clumpy structure of two spiral galaxies NGC 3184 (SAB(rs)cd HII) and NGC 3938 (SA(s)c HII) is analyzed at dierent wavelengths (8 and 24 Mm, NUV, H , and CO) using an algorithm called \Clump nd2d" (Williams et al. 1994). Based on the clumps found by this algorithm, the star formation rates (SFR)...
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| Udgivet i: | Revista Mexicana de Astronomía y Astrofísica |
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| Principais autores: | , |
| Format: | Artigo |
| Sprog: | Inglês |
| Udgivet: |
Universidad Nacional Autónoma de México
2008
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| Online adgang: | https://www.redalyc.org/articulo.oa?id=57116170027 |
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