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Molecular shock tracers in NGC?1068: SiO and HNCO

机译:NGC?1068中的分子冲击示踪剂:SiO和HNCO

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Aims. We present and compare the distribution of two shock tracers, SiO and HNCO, in the circumnuclear disk (CND) of NGC?1068. We aim to determine the causes of the variation in emission across the CND. Methods. SiO (3?2) and HNCO (6?5) emission has been imaged in NGC?1068 with the Plateau de Bure Interferometer (PdBI). We perform an LTE and RADEX analysis to determine the column densities and physical characteristics of the gas emitting these two lines. We then use a chemical model to determine the origin of the emission. Results. There is a strong SiO peak to the east of the AGN, with weak detections to the west. This distribution contrasts that of HNCO, which is detected more strongly to the west. The SiO emission peak in the east is similar to the peak of the molecular gas mass traced by CO. HNCO emission is offset from this peak by as much as ~ 80 pc ( hbox{$leqslant$} 1 ′′ ). We compare velocity integrated line ratios in the east and west. We confirm that SiO emission strongly dominates in the east, while the reverse is true in the west. We use RADEX to analyse the possible gas conditions that could produce such emission. We find that, in both east and west, we cannot constrain a single temperature for the gas. We run a grid of chemical models of potential shock processes in the CND and find that SiO is significantly enhanced during a fast (60 km?s ~(-1) ) shock but not during a slow (20 km?s ~(-1) ) shock, nor in a gas not subjected to shocks at all. We find the inverse for HNCO, whose abundance increases during slow shocks and in warm non-shocked gas. Conclusions. High SiO and low HNCO indicated a fast shock, while high HNCO and low SiO indicates either a slow shock or warm, dense, non-shocked gas. The East Knot is therefore likely to contain gas that is heavily shocked. From chemical modelling, gas in the West Knot may be non-shocked, or maybe undergoing a much milder shock event. When taking into account RADEX results, the milder shock event is the more likely of the two scenarios.
机译:目的我们提出并比较了两种冲击示踪剂SiO和HNCO在NGC?1068的核周盘中的分布。我们旨在确定导致整个CND排放变化的原因。方法。 SiO(3?2)和HNCO(6?5)的发射已通过Plateau de Bure干涉仪(PdBI)在NGC?1068中成像。我们执行LTE和RADEX分析,以确定发射这两条线的气体的色谱柱密度和物理特性。然后,我们使用化学模型来确定排放源。结果。在AGN的东部有一个很强的SiO峰,而在西部的探测却很弱。这种分布与HNCO的分布形成对比,后者在西方被更强烈地检测到。东部的SiO排放峰与CO跟踪的分子气体质量峰相似。HNCO排放与该峰的偏移量约为80 pc( hbox {$ leqslant $} 1′')。我们比较了东西方的速度积分线比率。我们确认,在东部,SiO的排放量占主导地位,而在西部,则相反。我们使用RADEX分析可能产生这种排放的气体条件。我们发现,在东西方,我们都不能限制气体的单一温度。我们在CND中运行了潜在冲击过程的化学模型网格,发现SiO在快速(60 km?s〜(-1))冲击过程中显着增强,而在慢速(20 km?s〜(-1)冲击中则没有增强))震动,也不要在根本不遭受震动的气体中。我们发现HNCO的倒数,在缓慢的冲击和温暖的非冲击气体中,其含量会增加。结论。高SiO和低HNCO表示快速震动,而高HNCO和低SiO表示缓慢震动或温暖,浓密,无冲击的气体。因此,“东结”很可能包含受到严重冲击的气体。通过化学建模,“西结”中的天然气可能不会受到电击,或者可能遭受的冲击要轻得多。考虑到RADEX的结果,在两种情况下,发生轻度冲击事件的可能性更高。

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