MASS DISTRIBUTION IN FLATTENED GALAXIES

被引：0

作者：

Bratek, L. ^{[1
]}

Jalocha-Bratek, J. ^{[1
]}

Kutschera, M. ^{[1
]}

机构：

[1] Polish Acad Sci, H Niewodniczanski Inst Nucl Phys, PL-31342 Krakow, Poland

来源：

ROLE OF THE DISK-HALO INTERACTION IN GALAXY EVOLUTION: OUTFLOWS VS INFALL? | 2012年 / 56卷

关键词：

MATTER;

D O I：

10.1051/eas/1256016

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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

引用

页码：119 / 123

页数：5

共 5 条

[1]

Binney J., 1987, GALACTIC DYNAMICS

[2] On the axisymmetric thin disc model of flattened galaxies [J].

Bratek, Lukasz ;

Jalocha, Joanna ;

Kutschera, Marek .

Jalocha, Joanna ;

Bratek, Lukasz ;

Kutschera, Marek .

[4]

Ryzhik I. M., 1951, TABLES INTEGRALS SUM

[5] ON DISTRIBUTION OF MATTER WITHIN HIGHLY FLATTENED GALAXIES [J].

TOOMRE, A .