The thickness of the HI gas layer in spiral galaxiesSicking, F. J., 1997, s.n..
Research output: Thesis › Thesis fully internal (DIV) › Academic
In the present study, in two inclined spiral galaxies, NGC 3198 and NGC 2403, the HI random velocity dispersion and layer thickness will be measured simultaneously. This will be done from the HI velocity dispersion field (the distribution on the sky of the observed HI line of sight velocity dispersion).
|Qualification||Doctor of Philosophy|
|Publication status||Published - 1997|
- Proefschriften (vorm), Waterstof, Interstellair gas, Spiraalnevels, 39.41
No data available