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首页> 外文期刊>The Astrophysical journal >Decreasing Density Gradients in Circumnuclear H?II Regions of Barred Galaxies NGC 1022, NGC 1326, and NGC 4314
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Decreasing Density Gradients in Circumnuclear H?II Regions of Barred Galaxies NGC 1022, NGC 1326, and NGC 4314

机译:禁止星系NGC 1022,NGC 1326和NGC 4314的核周H?II区的密度梯度减小

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A reanalysis of the radio continuum emission from circumnuclear regions of the barred galaxies NGC 1022, NGC 1326, and NGC 4314 is presented. The spatial distributions of Hα and radio continuum are similar and suggest the existence of several giant H II regions in the circumnuclear zone. The spectral indices of the H II regions, obtained with similar angular resolution and at three different wavelengths, indicate that in all three galaxies α -0.1. This result suggests the existence of giant H II regions with decreasing density gradients. The average density stratifications of these H II regions could be approximated by power laws of the form ne ∝ r-ω, with exponents in the range 1.6 ω 2.4.
机译:提出了对禁止星系NGC 1022,NGC 1326和NGC 4314周围核区域的无线电连续辐射的重新分析。 Hα和射电连续体的空间分布相似,表明在核周区域中存在几个巨大的H II区。以相似的角分辨率和在三个不同的波长获得的H II区的光谱指数表明,在所有三个星系中,α> -0.1。该结果表明存在密度梯度减小的巨型H II区。这些H II区的平均密度分层可以通过ne ∝r-ω形式的幂定律近似,指数范围为1.6 <ω<2.4。

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