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On the radio continuum, molecular gas content and optical emission of Markarian galaxies with Seyfert nuclei

机译：在核细胞中的无线电连续体，分子气体含量和甲状腺星系的光学发射

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In this paper we interpret C and X-band radio continuum observations of a sample of Markarian galaxies. The results are briefly discussed, Seyfert 2 galaxies show sistematically higher HI mass-to-blue magnitude than Seyfert 1 galaxies, as well as higher radio to fai-infiared luminosities The observational properties are interpreted in terms of simple non-thermal and dust emission. We obtained radio brightness temperatures, equipartion magnetic fields and total magnetic densities for the disks Upper limits for thermal densities are derived from simple free-free emission Star formation rates and mean supernova rates are estimated for individual Markarian galaxies The SFR values of the most luminous Markarian galaxies are considerably higher than those found in compact blue dwarf galaxies and also in gas-rich, early-type spirals.
机译：在本文中，我们解释了C和X波段无线电连续的标志性星系样本。简要讨论了结果，SEYFERT 2星系在SISTemize上展示了比SEYFERT 1星系的高度质量到蓝色幅度，以及较高的无线电到FIA-Indiate发光，在简单的非热和粉尘发射方面解释了观测性质。我们获得了无线电亮度温度，磁盘的磁盘磁场和总磁密度的热密度的上限来自于简单的无自由排放星形成速率，并且估计各个标记星系的平均超新星率最明显的标志性的SFR值星系比在紧凑型蓝矮星系中发现的星系以及富含气体早期螺旋的星系。

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