| タイトル | Far-infrared observations of two southern H II regions - RCW 122 and G 351.6-1.3 |
| 著者（英） | Rengarajan, T. N.; Mcbreen, B.; Fazio, G. G.; Loughran, L. |
| 著者所属（英） | Harvard-Smithsonian Center for Astrophysics|University Coll.|Tata Inst. of Fundamental Research |
| 発行日 | 1985-01-01 |
| 言語 | eng |
| 内容記述 | The luminosities in excess of 1,000,000 solar luminosities obtained in the present 1-arcmin resolution mapping of the two southern H II regions RCW 122 and G 351.6-1.3 requires the presence of OB star clusters. A luminosity/unit mass of the associated cloud of about 6 solar luminosities/solar mass is obtained by combining near-IR, far-IR, and CO-emission properties for RCW 122, and it is determined that the emitting dust grains are amorphous silicate-like. G 351.6-1.3 has very similar properties, although the fraction of 1-25 micron luminosity corrected for silicate absorption is about five times less than for RCW 122. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 85A21711 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/393249 |
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