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Mass distribution in flattened galaxies

Published online by Cambridge University Press:  17 September 2012

Ł. Bratek ,
J. Jałocha-Bratek  and
M. Kutschera
Ł. Bratek
Affiliation:
H. Niewodniczański Institute of Nuclear Physics, Polish Academy of Sciences, Radzikowskego 152, 31342 Kraków, Poland. e-mail: Joanna.Jalocha@ifj.edu.pl;
J. Jałocha-Bratek
Affiliation:
H. Niewodniczański Institute of Nuclear Physics, Polish Academy of Sciences, Radzikowskego 152, 31342 Kraków, Poland. e-mail: Joanna.Jalocha@ifj.edu.pl;
M. Kutschera
Affiliation:
H. Niewodniczański Institute of Nuclear Physics, Polish Academy of Sciences, Radzikowskego 152, 31342 Kraków, Poland. e-mail: Joanna.Jalocha@ifj.edu.pl; M. Smoluchowski Institute of Physics, Jagellonian University, Reymonta 4, 30059 Kraków, Poland
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Abstract

It is shown that mass distribution of baryonic matter accounts for the rotation curve of galaxy NGC 4736.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 56: The Role of the Disk-Halo Interaction in Galaxy Evolution: Outflow vs. Infall? , 2012 , pp. 119 - 123
Copyright
© EAS, EDP Sciences, 2012

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References

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