| タイトル | IRAS observations of Shapley-Ames galaxies |
| 著者（英） | Houck, J. R.; Aumann, H. H.; De Jong, T.; Rowan-Robinson, M.; Soifer, B. T.; Clegg, P. E.; Raimond, E.; Habing, H. J. |
| 著者所属（英） | Cornell Univ.|Jet Propulsion Lab., California Inst. of Tech.|Leiden Univ.|Amsterdam Univ.|London Univ.|California Inst. of Tech.|Radio Sterrenwacht |
| 発行日 | 1984-03-01 |
| 言語 | eng |
| 内容記述 | A preliminary discussion of the infrared properties of a representative subsample of galaxies in the Revised Shapley-Ames Catalog (B less than about 13 mag) is presented. Of the 165 galaxies in the sample, 108 predominantly spiral galaxies, are detected in the infrared by IRAS. None of the elliptical galaxies and only about 25 percent of the lenticular galaxies scanned were detected. The range of infrared-to-blue luminosity ratios, a measure of the infrared excess of galaxies, is large, varying from roughly 0.1 to roughly 5. The data suggest that weakly infrared emitting galaxies are cool (100-60 micron color temperatures of about 25 K), while the more infrared luminous ones tend to be warmer (about 50 K). The rate of star formation in barred spiral galaxies is apparently higher than in normal spirals. About 1 solar mass/year of interstellar matter is converted into massive stars in the typical spiral galaxy. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 84A27715 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/398876 |
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