A Tail of Two Clumps

Author:

Raga Alejandro Cristian,Cantó Jorge,Castellanos-Ramírez Antonio,Castorena Jorge Ivan,Hernández-Martínez LilianaORCID,Rodríguez-González Ary,Rivera-Ortíz Pedro

Abstract

We present two axisymmetric simulations of a high velocity clump in a photoionized region: one for the case of a uniform, low density environment and a second one for the case of a clump first traveling within a high density medium and then emerging into a low density environment. We show that the second scenario results in the production of an axial tail of dense material with a linear velocity vs. position ramp (with zero velocity at the high/low density environment transition). This material comes from a confined bow shock (produced by the clump when it was within the dense cloud) that emerges into the low environmental density region.

Publisher

MDPI AG

Subject

Astronomy and Astrophysics

Cited by 1 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Modelling the CO streamers in the explosive ejection of Orion BN/KL region;Monthly Notices of the Royal Astronomical Society;2022-12-28

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