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
Hauptverfasser: Blaauw, A., Fejes, I., Tolbert, C. R., Hulsbosch, A. N. M., Raimond, E.
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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.
ISSN:0074-1809
DOI:10.1017/S0074180900101068