The Infall of the Virgo Elliptical Galaxy M60 toward M87 and the Gaseous Structures Produced by Kelvin-Helmholtz Instabilities
arXiv:1703.05883 · doi:10.3847/1538-4357/aa8723
Abstract
We present Chandra observations of hot gas structures, characteristic of gas stripping during infall, in the Virgo cluster elliptical galaxy M60 (NGC4649) located Mpc east of M87. keV Chandra X-ray images show a sharp leading edge in the surface brightness kpc north and west of the galaxy center in the direction of M87 characteristic of a merger cold front due to M60's motion through the Virgo ICM. We measured a temperature of keV for abundance inside the edge and keV for abundance in the Virgo ICM free stream region. We find that the observed jump in surface brightness yields a density ratio of between gas inside the edge and in the cluster free stream region. If the edge is a cold front due solely to the infall of M60 in the direction of M87, we find a pressure ratio of and Mach number . For 1.37 keV Virgo gas we find a total infall velocity for M60 of kms. We calculate the motion in the plane of the sky to be km implying an inclination angle degrees. Surface brightness profiles show the presence of a faint diffuse gaseous tail. We identify filamentary, gaseous wing structures caused by the galaxy's motion through the ICM. The structure and dimensions of these wings are consistent with simulations of Kelvin-Helmholtz instabilities as expected if the gas stripping is close to inviscid.
arXiv comment12 pages, 7 figures, added references, discussion of magnetic fields and other minor text changes to conform to published version, results unchanged
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