| タイトル | The structure of galactic HI in directions of low total column density |
| 本文（外部サイト） | http://hdl.handle.net/2060/19850019473 |
| 著者（英） | Lockman, F. J.; Mccammon, D.; Jahoda, K. |
| 著者所属（英） | National Radio Astronomy Observatory |
| 発行日 | 1985-01-01 |
| 言語 | eng |
| 内容記述 | A detailed 21 cm study of areas of that have the smallest known amount of HI in the northern sky was performed. These observations were corrected for stray radiation. The region of main interest, around alpha = 10(h)45(m), delta = 57 deg 20', has a minimium N(HI) of 4.5 x 10 to the 19th power/sq cm. Spectra taken at 21' resolution over a field 4 x 3 deg in this direction show up to four HI line components. Two, near 0 and -50 km/s, are ubiquitous. There is also a narrow component at -10 km/s attributable to a diffuse cloud covering half of the field, and scattered patches of HI at v -100 km/s. the low and intermediate velocity components have a broad line width and are so smoothly distributed across the region that it is unlikely that they contain significant unresolved angular structure. Eight other low column density directions were also observed. Their spectra typically have several components, but the total column density is always 7 x 10 to the 19th power/sq cm and changes smoothly along a 2 deg strip. Half of the directions show narrow lines arising from weak diffuse HI clouds that contain 0.5 to 3.0 x 10 to the 19th power/sq cm. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 85N27785
NASA-CR-175709
NAS 1.26:175709 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/156294 |
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