International audienceThis is the first paper of a series in which we will attempt to put constraints on the flattening of dark halos in disk galaxies. We observe for this purpose the HI in edge-on galaxies, where it is in principle possible to measure the force field in the halo vertically and radially from gas layer flaring and rotation curve decomposition respectively. In this paper, we define a sample of 8 HI rich late-type galaxies suitable for this purpose and present the HI observations
This is the second paper of a series in which we attempt to put constraints on the flattening of dar...
In a previous paper (Olling 1995, astro-ph/9505002) a method was developed to determine the shapes o...
International audienceThe HI in disk galaxies frequently extends beyond the optical image and can tr...
International audienceThis is the first paper of a series in which we will attempt to put constraint...
This is the first paper of a series in which we will attempt to put constraints on the flattening of...
This is the third paper in a series in which we attempt to put constraints on the flattening of dark...
This is the third paper in a series in which we attempt to put constraints on the flattening of dark...
This is the second paper of a series in which we attempt to put constraints on the flattening of dar...
The shape of the dark matter halo of a galaxy offers valuable clues on the physical nature of dark m...
This is the fourth paper in a series in which we attempt to put constraints on the flattening of dar...
This is the fourth paper in a series in which we attempt to put constraints on the flattening of dar...
In previous papers in this series, we measured the stellar and HI content in a sample of edge-on gal...
This is the third paper in a series in which we attempt to put constraints on the flattening of dark...
This is the second paper of a series in which we attempt to put constraints on the flattening of dar...
In a previous paper (Olling 1995, astro-ph/9505002) a method was developed to determine the shapes o...
International audienceThe HI in disk galaxies frequently extends beyond the optical image and can tr...
International audienceThis is the first paper of a series in which we will attempt to put constraint...
This is the first paper of a series in which we will attempt to put constraints on the flattening of...
This is the third paper in a series in which we attempt to put constraints on the flattening of dark...
This is the third paper in a series in which we attempt to put constraints on the flattening of dark...
This is the second paper of a series in which we attempt to put constraints on the flattening of dar...
The shape of the dark matter halo of a galaxy offers valuable clues on the physical nature of dark m...
This is the fourth paper in a series in which we attempt to put constraints on the flattening of dar...
This is the fourth paper in a series in which we attempt to put constraints on the flattening of dar...
In previous papers in this series, we measured the stellar and HI content in a sample of edge-on gal...
This is the third paper in a series in which we attempt to put constraints on the flattening of dark...
This is the second paper of a series in which we attempt to put constraints on the flattening of dar...
In a previous paper (Olling 1995, astro-ph/9505002) a method was developed to determine the shapes o...
International audienceThe HI in disk galaxies frequently extends beyond the optical image and can tr...