首页> 外文会议>International Astronomical Union., Symposium;Symposium of the International Astronomical Union >Diving deeper into jellyfish: The rich population of jellyfish galaxies in Abell 901/2
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Diving deeper into jellyfish: The rich population of jellyfish galaxies in Abell 901/2

机译:深入潜水到水母:富裕人口富含牛奶鲸星系的阿伯塞尔901/2

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Jellyfish galaxies are the most extreme examples of ram pressure stripping (RPS). They represent an important path in the morphological change and quenching in galaxy clusters, however they are still not well characterised morphologically and finding them is a complex task based mainly on visual inspection. We present a study on the properties of a large sample of jellyfish candidates in the multi-cluster system A901/2. We find evidence that the multi-cluster is triggering RPS events in preferential regions in the system and that these galaxies have enhanced specific star formation rates. We also use the software Morfometryka in order to analyse the unique morphometric features in jellyfish galaxies providing a better comprehension of their physical state and future. This can help unravel the physical processes behind such extreme morphologies as well as possibly automatising the search for jellyfish galaxy candidates in large surveys in the next era of instruments.
机译:水母星系是RAM压力剥离(RPS)最极端的例子。 它们代表了在星系集群中的形态变化和淬火中的重要路径,但它们仍然没有很好地在形态学上表征,并发现它们是一个主要基于目视检查的复杂任务。 我们在多簇系统A901 / 2中展示了大型水母候选的大型样品的性质。 我们发现多集群在系统中优先区域中触发RPS事件,这些星系具有增强的特定恒星形成率。 我们还使用软件Morfomfortka,以分析水母星系中的独特形态学特征,提供更好地理解其物理状态和未来。 这可以帮助解开这种极端形态背后的物理过程,以及可能在下一个仪器中的大型调查中自动化了对水母星系候选的搜索。

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