A new way to constrain the densities of intragroup medium in groups of galaxies with convolutional neural networks
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DOI: 10.1093/mnras/staa2226
Abstract: Ram pressure (RP) can influence the evolution of cold gas content and star formation rates of galaxies. One of the key parameters for the strength of RP is the density of intra-group medium ($\rho_{\rm igm}$),… read more here.
Keywords: rho igm; neural networks; convolutional neural; new way ... See more keywords