Motions of neutral hydrogen at high latitudes
Earlier investigations have shown that there is a preponderance of negative velocities in the hydrogen gas at high latitudes, and that in certain areas very little low-velocity gas occurs. In the region 100° < l < 250°, + 40° < b < + 85°, there appears to be a disturbance, with velocitie...
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Veröffentlicht in: | Symposium - International Astronomical Union 1967, Vol.31, p.265-278 |
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Format: | Artikel |
Sprache: | eng |
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Zusammenfassung: | Earlier investigations have shown that there is a preponderance of negative velocities in the hydrogen gas at high latitudes, and that in certain areas very little low-velocity gas occurs. In the region 100° <
l
< 250°, + 40° <
b
< + 85°, there appears to be a disturbance, with velocities between - 30 and - 80 km/sec. This ‘streaming’ involves about 3000 (
r
/100)
2
solar masses (
r
in pc). In the same region there is a low surface density at low velocities (|
V
| < 30 km/sec). About 40% of the gas in the disturbance is in the form of separate concentrations superimposed on a relatively smooth background. The number of these concentrations as a function of velocity remains constant from - 30 to - 60 km/sec but drops rapidly at higher negative velocities. The velocity dispersion in the concentrations varies little about 6·2 km/sec. Concentrations at positive velocities are much less abundant. |
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ISSN: | 0074-1809 |
DOI: | 10.1017/S0074180900101068 |