Add to ORKGA brief overview is presented of some results from ongoing research on the properties of a complete sample of spiral galaxies in the Ursa Major cluster. Optical and near infrared photometric imaging is combined with HI 21cm-line synthesis mapping. These observations allow to study in great detail the Tully-Fisher relations in various passbands with different kinematic measures and to investigate the properties of the dark matter halos as a function of the global properties of the luminous matter.</p
A systematic variation of the dark matter abundance in spiral galaxies, previously reported (Persic ...
A systematic variation of the dark matter abundance in spiral galaxies, previously reported (Persic ...
We use a homogeneous sample of about 1100 optical and radio rotation curves (RCs); and relative surf...
A brief overview is presented of some results from ongoing research on the properties of a complete ...
In this data paper we present the results of an extensive 21 cm-line synthesis imaging survey of 43 ...
In this data paper we present the results of an extensive 21 cm-line synthesis imaging survey of 43 ...
We present new magnitudes derived from 1.65 mum images for 23 galaxies in the Ursa Major cluster. Ma...
The Tully-Fisher relation is used to probe dark matter (DM) in the optical regions of spiral galaxie...
This is a progress report on a survey of detailed HI synthesis observations of galaxies in the Ursa ...
The Tully-Fisher (TF) relation is an empirically establish correlation between the luminosity of a s...
We construct mass models of 28 S0-Sb galaxies. The models have an axisymmetric stellar component and...
Submitted to: Astrophys. J. Abstract: The Ursa Major Cluster appears to be unevolved and made up of ...
The research presented in this Ph.D thesis is mainly focused on the Tully– Fisher relation as a tool...
The properties of molecular gas in spiral galaxies is the subject of a wide field of research and mu...
We present new magnitudes derived from 1.65 micron images for 23 galaxies in the Ursa Major cluster....
A systematic variation of the dark matter abundance in spiral galaxies, previously reported (Persic ...
A systematic variation of the dark matter abundance in spiral galaxies, previously reported (Persic ...
We use a homogeneous sample of about 1100 optical and radio rotation curves (RCs); and relative surf...
A brief overview is presented of some results from ongoing research on the properties of a complete ...
In this data paper we present the results of an extensive 21 cm-line synthesis imaging survey of 43 ...
In this data paper we present the results of an extensive 21 cm-line synthesis imaging survey of 43 ...
We present new magnitudes derived from 1.65 mum images for 23 galaxies in the Ursa Major cluster. Ma...
The Tully-Fisher relation is used to probe dark matter (DM) in the optical regions of spiral galaxie...
This is a progress report on a survey of detailed HI synthesis observations of galaxies in the Ursa ...
The Tully-Fisher (TF) relation is an empirically establish correlation between the luminosity of a s...
We construct mass models of 28 S0-Sb galaxies. The models have an axisymmetric stellar component and...
Submitted to: Astrophys. J. Abstract: The Ursa Major Cluster appears to be unevolved and made up of ...
The research presented in this Ph.D thesis is mainly focused on the Tully– Fisher relation as a tool...
The properties of molecular gas in spiral galaxies is the subject of a wide field of research and mu...
We present new magnitudes derived from 1.65 micron images for 23 galaxies in the Ursa Major cluster....
A systematic variation of the dark matter abundance in spiral galaxies, previously reported (Persic ...
A systematic variation of the dark matter abundance in spiral galaxies, previously reported (Persic ...
We use a homogeneous sample of about 1100 optical and radio rotation curves (RCs); and relative surf...