Intracluster Shocking of the ISM in Virgo Cluster Spirals: Modified FIR-Radio Relations
Eric Murphy (IPAC)
We present a study on the effects of the intracluster medium (ICM) on the interstellar medium (ISM) of 10 Virgo cluster galaxies using Spitzer far-infrared (FIR) and VLA radio continuum imaging. Relying on the FIR-radio correlation within normal galaxies, we use our infrared data to create model radio maps which we compare to the observed radio images. For 6 of our sample galaxies we find regions along their outer edges that are highly deficient in the radio compared with our models. We believe these observations are the signatures of ICM ram pressure. For NGC~4522 we find the radio deficit region to lie just exterior to a region of high radio polarization and flat radio spectral index, although the total 20~cm radio continuum in this region does not appear strongly enhanced. This scenario seems consistent for other galaxies with radio polarization data in the literature. Using the deficit region as a measure for the strength of the current ongoing ram pressure, we find it to be proportional to the time since peak pressure as inferred by stellar population studies and gas stripping simulations. We also find that galaxies having local radio deficits appear to have enhanced global radio fluxes. Our preferred physical picture is that the observed radio deficit regions arise from the ICM wind sweeping away cosmic-ray (CR) electrons and the associated magnetic field, thereby creating synchrotron tails as observed for some of our galaxies. We propose that CR particles are also re-accelerated by ICM-driven shocklets behind the observed radio deficit regions which in turn enhances the remaining radio disk brightness. The high radio polarization and lack of precisely coincident enhancement in the total synchrotron power for these regions suggests shearing, and possibly mild compression of the magnetic field, as the ICM wind drags and stretches the leading edge of the ISM.
Host: Barry Madore
Eric Murphy (IPAC)
We present a study on the effects of the intracluster medium (ICM) on the interstellar medium (ISM) of 10 Virgo cluster galaxies using Spitzer far-infrared (FIR) and VLA radio continuum imaging. Relying on the FIR-radio correlation within normal galaxies, we use our infrared data to create model radio maps which we compare to the observed radio images. For 6 of our sample galaxies we find regions along their outer edges that are highly deficient in the radio compared with our models. We believe these observations are the signatures of ICM ram pressure. For NGC~4522 we find the radio deficit region to lie just exterior to a region of high radio polarization and flat radio spectral index, although the total 20~cm radio continuum in this region does not appear strongly enhanced. This scenario seems consistent for other galaxies with radio polarization data in the literature. Using the deficit region as a measure for the strength of the current ongoing ram pressure, we find it to be proportional to the time since peak pressure as inferred by stellar population studies and gas stripping simulations. We also find that galaxies having local radio deficits appear to have enhanced global radio fluxes. Our preferred physical picture is that the observed radio deficit regions arise from the ICM wind sweeping away cosmic-ray (CR) electrons and the associated magnetic field, thereby creating synchrotron tails as observed for some of our galaxies. We propose that CR particles are also re-accelerated by ICM-driven shocklets behind the observed radio deficit regions which in turn enhances the remaining radio disk brightness. The high radio polarization and lack of precisely coincident enhancement in the total synchrotron power for these regions suggests shearing, and possibly mild compression of the magnetic field, as the ICM wind drags and stretches the leading edge of the ISM.
Host: Barry Madore