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Gas inflow and nuclear star formation in galaxies with non-axisymmetric bulges

机译:燃气流入和核星形成具有非轴对称凸起的星系中

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We present the dependence of the amount of nuclear star formation on the non-axisymmetry of a bulge of disk galaxies. For this, we use a volume-limited sample of spiral galaxies at 0.02 <= z < 0.055 from the SDSS DR7. Among 3173 final sample galaxies with an axis ratio b/a > 0.6 and a bulge fraction ranged in B/T <= 0.41, nuclear starburst galaxies are 10 %. We find that a fraction of the nuclear starburst galaxies become higher when ellipticity of a bulge increases in early type galaxies. Also, the fraction increases clearly when early type galaxies are isolated and in low density region. Our results indicate that the non-axisymmetry of bulges assists gas to fall inside and affects the nuclear starburst process in disk galaxies.
机译:我们呈现核星形成量对盘星形膨胀的非轴对称的依赖性。为此,我们使用从SDSS DR7的0.02 <= Z <0.055的螺旋星系的体积限制样品。在3173个最终样品星系中,具有轴比的B / A> 0.6和B / T <= 0.41的凸起分数,核爆炸星系是10%。我们发现,当早期星系的抗凸起的椭圆增加增加时,核爆炸星系的一部分变得更高。而且,当早期的星系是隔离和低密度区域时,分数显然增加。我们的结果表明,凸起的非轴对称助攻气体落入内部,并影响磁盘星系中的核爆炸过程。

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