| タイトル | The binary system MWC 349 |
| 著者（英） | Dreher, J. W.; Bieging, J. H.; Welch, W. J.; Cohen, M. |
| 著者所属（英） | NASA Ames Research Center|California Univ.|Massachusetts Inst. of Tech. |
| 発行日 | 1985-05-01 |
| 言語 | eng |
| 内容記述 | The ionized zone surrounding MWC 349 has been resolved using the VLA. On the basis of a radio continuum map, it is concluded that there is a physical interaction between the two stellar components of MWC 349, and that the system is therefore a binary. The B component can be classified as a B0 III star, yielding a distance of about 1.2 kpc for the binary. The low ratio of infrared to short-wavelength luminosity in the A component suggests a circumstellar dusty region of special geometry. It is proposed that an appreciable dust and gas disk surrounds the star, modifying the symmetry of its H II region, and yielding the low infrared luminosity and perhaps its extra circumstellar extinction. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 85A35429 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/391303 |
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