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Multicolor CCD photometry of six lenticular and spiral galaxies. Structure of the galaxies

机译:六个透镜状和螺旋状星系的多色CCD光度法。星系的结构

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摘要

The results Of multicolor Surface photometry of the S0 galaxies NGC 524, NGC 1138, and NGC 7280 and the spiral galaxies NGC 532, NGC 783, and NGC 1589 are reported. UBV RI observations were acquired with the 1.5-m telescope of the Maidanak Observatory (Uzbekistan), while JHK data were taken from the 2MASS catalog. The overall structure of the galaxies is analyzed and the galaxy images decomposed into bulge and disk components. The parameters of the galaxy components-rings, bars, spiral arms, and dust lanes-are determined. The bulge/disk decompositions based on averaged one-dimensional photometric profiles yield incorrect parameters for the bulges Of the S0-Sa galaxies with bars aud/or rings, whose inner regions are dominated by the radiation of the bulge.
机译:报告了S0星系NGC 524,NGC 1138和NGC 7280以及旋涡星系NGC 532,NGC 783和NGC 1589的多色表面光度法的结果。 UBV RI观测是通过Maidanak天文台(乌兹别克斯坦)的1.5米望远镜获得的,而JHK的数据则来自2MASS目录。分析了星系的整体结构,并将星系图像分解为凸起和盘状成分。确定了银河系组件的参数,包括环,条,螺旋臂和尘埃带。基于平均一维光度轮廓的凸起/圆盘分解会产生带有aud //或bar环的S0-Sa星系的凸起的不正确参数,其内部区域由凸起的辐射决定。

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