| タイトル | Submillimeter wavelength survey of the galactic plane from l = -5 deg to l = +62 deg - Structure and energetics of the inner disk |
| 著者（英） | Silverberg, R. F.; Gezari, D. Y.; Dwek, E.; Kelsall, T.; Hauser, M. G.; Walser, D.; Cheung, L. H.; Mather, J. C.; Stier, M. T. |
| 著者所属（英） | Maryland Univ.|NASA Goddard Space Flight Center |
| 発行日 | 1984-10-01 |
| 言語 | eng |
| 内容記述 | Observational results are presented from a new large-scale survey of the first quadrant of the galactic plane at wavelengths of 150, 250, and 300 microns, with a 10 x 10 arcmin beam. The emission detected in the survey arises from compact sources, most of which are identified with known peaks of 5 GHz or CO emission, or both, and from an underlying diffuse background with a typical angular width of about 0.9 deg (FWHM) which accounts for most of the emission. A total of 80 prominent discrete sources are identified and characterized, of which about half have not previously been reported at far-infrared wavelengths. The total infrared luminosity within the solar circle is about 1 to 2 x 10 to the 10th solar luminosity, and is probably emitted by dust that resides in molecular clouds. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 85A13834 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/394268 |
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