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Ultraviolet-optical observations of the Seyfert 2 galaxies NGC 7130, NGC 5135, and IC 3639: implication for the starburst-active galactic nucleus connection

机译:Seyfert 2星系NGC 7130,NGC 5135和IC 3639的紫外光学观察:对星暴活动的银河核连接的暗示

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摘要

We present and discuss Hubble Space Telescope(HST)(WFPC2 and FOC) images and ultraviolet (GHRS) spectra plus ground-based optical spectra of three Seyfert 2 nuclei(NGC 7130 NGC 5135 and IC 3639). These galaxies, together with Mrk 477 (Heckman et al.), were selected on the basis of ultravio- let brightness from a bigger sample that comprises the 20 brightest Seyfert 2 nuclei, with the goal of Studying the starburst-active galactic nucleus (AGN) connection and the origin of the so-called "featureless continuum" in Seyfert 2 nuclei.
机译:我们介绍并讨论了哈勃太空望远镜(HST)(WFPC2和FOC)的图像和紫外(GHRS)光谱以及三个塞弗2核(NGC 7130 NGC 5135和IC 3639)的地基光谱。这些星系与Mrk 477(Heckman等人)是根据包含20个最亮Seyfert 2核的较大样本的紫外线亮度选择的,目的是研究星爆活性星系核(AGN)。 )连接和塞弗特2核中所谓的“无特征连续体”的起源。

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