| Issue |
EAS Publications Series
Volume 56, 2012
The Role of the Disk-Halo Interaction in Galaxy Evolution: Outflow vs. Infall?
|
|
|---|---|---|
| Page(s) | 119 - 123 | |
| Section | The ISM in Distant Galaxies | |
| DOI | https://doi.org/10.1051/eas/1256016 | |
| Published online | 17 September 2012 | |
The Role of the Disk-Halo Interaction in Galaxy Evolution: Outflow vs. Infall?
Miguel A. de Avillez (ed)
EAS Publications Series, 56 (2012) 119–123
Miguel A. de Avillez (ed)
EAS Publications Series, 56 (2012) 119–123
Mass distribution in flattened galaxies
1 H. Niewodniczański Institute of Nuclear Physics, Polish Academy of Sciences, Radzikowskego 152, 31342 Kraków, Poland ;
e-mail: Joanna.Jalocha@ifj.edu.pl
2 M. Smoluchowski Institute of Physics, Jagellonian University, Reymonta 4, 30059 Kraków, Poland
It is shown that mass distribution of baryonic matter accounts for the rotation curve of galaxy NGC 4736.
© EAS, EDP Sciences, 2012