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New H I-detected Galaxies in the Zone of Avoidance

机译:新的H I探测到的回避星系

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We present the first results of a blind H I survey for galaxies in the southern zone of avoidance with a multibeam receiver on the Parkes telescope. This survey is expected to eventually catalog several thousand galaxies within Galactic latitude |b| 5°, mostly unrecognized before because of Galactic extinction and confusion. We present here the results of the first three detections to have been imaged with the Australia Telescope Compact Array. All the galaxies lie near Galactic longitude 325° and were selected because of their large angular sizes, up to 13. Linear sizes range from 53 to 108 kpc. The first galaxy is a massive 5.7 × 1011 M⊙ disk galaxy with a faint optical counterpart, SGC 1511.1-5249. The second is probably an interacting group of galaxies straddling the Galactic equator. No optical identification is possible. The third object appears to be an interacting pair of low column density galaxies, possibly belonging to an extended Circinus or Centaurus A galaxy group. No optical counterpart has been seen despite the predicted extinction (AB = 2.7–4.4 mag) not being excessive. We discuss the implications of the results, in particular, the low H I column densities (~1019 atoms cm-2) found for two of the three galaxies.
机译:我们用帕克斯望远镜上的多波束接收器介绍了对避免区域南部的星系进行盲目H I测量的初步结果。预计该调查最终将在银河纬度| b |内对数千个星系进行分类。 <5°,由于银河系的灭绝和混乱,以前大多无法识别。我们在这里展示了澳大利亚望远镜紧凑阵列成像的前三个检测结果。所有星系都位于银河经度325°附近,并且由于它们的大角度大小(最多13个)而被选中。线性大小范围从53到108 kpc。第一个星系是巨大的5.7×1011M⊙盘状星系,其光学对应物为SGC 1511.1-5249。第二个可能是横跨银河赤道的一组相互作用的星系。无法进行光学识别。第三个物体似乎是相互作用的一对低列密度星系,可能属于扩展的马戏团或半人马座A星系。尽管预计消光(AB = 2.7-4.4 mag)并不过度,但仍未见到任何光学对应物。我们讨论了结果的含义,特别是三个星系中两个星系的低H I列密度(〜1019原子cm-2)。

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