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ALMA evidence for ram pressure compression and stripping of molecular gas in the Virgo cluster galaxy NGC 4402 by Cramer, William J.; Kenney, Jeffrey D. P.; Cortes, Juan R.; Cortes, Paulo C.; Vlahakis, Catherine; Jáchym, Pavel; Pompei, Emanuela; Rubio, Monica is a scholarly article available to read on EtoBox.

What is ALMA evidence for ram pressure compression and stripping of molecular gas in the Virgo cluster galaxy NGC 4402 about?

High resolution (1'' $\times$ 2'') ALMA CO(2-1) observations of the ram pressure stripped galaxy NGC 4402 in the Virgo cluster show some of the clearest evidence yet for the impacts of ram pressure on the molecular ISM of a galaxy. The eastern side of the galaxy at $r \sim 4.5$ kpc, upon which ram pressure is incident, has a large (width $\sim$1 kpc, height $\sim$1 kpc above the disk midplane) extraplanar plume of molecular gas and dust. Molecular gas in the plume region shows distinct non-circular motions in the direction of the ram pressure; the kinematic offset of up to 60 km s$^{-1}$ is consistent with acceleration by ram pressure. We also detect a small amount of gas in clouds below the plume that are spatially and kinematically distinct from the surrounding medium, and appear to be decoupled from the stripped ISM. We propose that diffuse molecular gas is directly stripped but GMC density gas is not directly stripped, and so decouples from lower density stripped gas. However, GMCs become effectively stripped on short timescales. We also find morphological and kinematic signatures of ram pressure compression of molecular gas in a region of intense star formation on the leading

Author

Cramer, William J.; Kenney, Jeffrey D. P.; Cortes, Juan R.; Cortes, Paulo C.; Vlahakis, Catherine; Jáchym, Pavel; Pompei, Emanuela; Rubio, Monica

Published

2019

Language

EN