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A DEEP SEARCH FOR FAINT GALAXIES ASSOCIATED WITH VERY LOW-REDSHIFT C IV ABSORBERS: A CASE WITH COLD-ACCRETION CHARACTERISTICS

机译:深度搜索与非常低的微闪光C IV吸收剂相关的微弱星系:一种具有冷增值特性的情况

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摘要

Studies of QSO absorber–galaxy connections are often hindered by inadequate information on whether faint/dwarfgalaxies are located near the QSO sight lines. To investigate the contribution of faint galaxies to QSO absorberpopulations, we are conducting a deep galaxy redshift survey near low-z Civ absorbers. Here we report a blindlydetected C iv absorption system (zabs = 0.00348) in the spectrum of PG1148+549 that appears to be associatedeither with an edge-on dwarf galaxy with an obvious disk (UGC 6894, zgal = 0.00283) at an impact parameter ofρ = 190 kpc or with a very faint dwarf irregular galaxy at ρ = 23 kpc, which is closer to the sightline but has alarger redshift difference (zgal = 0.00107, i.e., δv = 724 km s−1). We consider various gas/galaxy associations,including infall and outflows. Based on current theoretical models, we conclude that the absorber is most likelytracing (1) the remnants of an outflow from a previous epoch, a so-called “ancient outflow”, or (2) intergalactic gasaccreting onto UGC 6894, “cold mode” accretion. The latter scenario is supported by Hi synthesis imaging datathat shows the rotation curve of the disk being codirectional with the velocity offset between UGC 6894 and theabsorber, which is located almost directly along the major axis of the edge-on disk.
机译:有关QSO视星线是否位于QSO视线附近的信息不足,通常会​​阻碍对QSO吸收器-星系连接的研究。为了研究微弱星系对QSO吸收体种群的贡献,我们正在低z Civ吸收体附近进行深层星系红移调查。在这里,我们报道了在PG1148 + 549光谱中被盲目检测到的Civ吸收系统(zabs = 0.00348),它似乎与边缘参数相近的矮星系具有明显的圆盘(UGC 6894,zgal = 0.00283),冲击参数为ρ = 190 kpc或在ρ= 23 kpc时有非常微弱的矮星不规则星系,它更靠近视线但具有较大的红移差(zgal = 0.00107,即δv= 724 km s-1)。我们考虑各种气体/星系的关联,包括流入和流出。根据当前的理论模型,我们得出的结论是,吸收器最有可能追查(1)从前一个时期流出的残余物,即所谓的“古代流出物”,或(2)吸收银河系气体进入UGC 6894的“冷态”积聚。后一种情况得到了Hi合成成像数据的支持,Hi合成成像数据显示了圆盘的旋转曲线与UGC 6894和吸收器之间的速度偏移同向,该速度偏移几乎直接沿着边缘在圆盘上的主轴线定位。

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