| タイトル | Far-infrared and CO observations of the W33 complex |
| 著者（英） | Fazio, G. G.; Maxson, C. W.; Sciortino, S.; Jaffe, D. T.; Mcbreen, B.; Rengarajan, T. N.; Stier, M. T.; Loughran, L.; Serio, S. |
| 著者所属（英） | California Univ.|University Coll.|Tata Inst. of Fundamental Research|Perkin-Elmer Corp.|Harvard-Smithsonian Center for Astrophysics|Osservatorio Astronomico |
| 発行日 | 1984-08-15 |
| 言語 | eng |
| 内容記述 | The giant H II region W33 is a strong radio continuum source. However, it has received little attention compared to the nearby M17 region. The present investigation is concerned with the results of 1 min resolution far-infrared (far-IR) and CO observations of the W33 region. The complex has been resolved into several components at the far-IR wavelengths, and information has been obtained regarding spectral characteristics in the range from 20 to 250 microns. An examination is conducted of the nature of the individual W33 sources and their relationship to the radio sources and the molecular clouds. Particular attention is given to the nature of the unusual source W33 A which has a very high ratio of far-IR to radio luminosity. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 84A47914 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/396373 |
|
