Direct Evidence for Outflow of Metal-enriched Gas Along the Radio Jets of Hydra A Export

@article{citeulike:5785379, abstract = {Using deep Chandra observations of the Hydra A galaxy cluster, we examine the metallicity structure near the central galaxy and along its powerful radio source. We show that the metallicity of the intracluster medium is enhanced by up to 0.2 dex along the radio jets and lobes compared to the metallicity of the undisturbed gas. The enhancements extend from a radius of 20 kpc from the central galaxy to a distance of \~{} 120 kpc. We estimate the total iron mass that has been transported out of the central galaxy to be between 2 x 10^7 M\_sun and 7 x 10^7 M\_sun which represents 10\% - 20\% of the iron mass within the central galaxy. The energy required to lift this gas is roughly 1\% to 5\% of the total energetic output of the AGN. Evidently, Hydra A's powerful radio source is able to redistribute metal-enriched, low entropy gas throughout the core of the galaxy cluster. The short re-enrichment time scale \< 10^9 yr implies that the metals lost from the central galaxy will be quickly replenished.}, archivePrefix = {arXiv}, author = {Kirkpatrick, C. C. and Gitti, M. and Cavagnolo, K. W. and McNamara, B. R. and David, L. P. and Nulsen, P. E. J. and Wise, M. W.}, citeulike-article-id = {5785379}, citeulike-linkout-0 = {http://arxiv.org/abs/0909.2252}, citeulike-linkout-1 = {http://arxiv.org/pdf/0909.2252}, day = {11}, eprint = {0909.2252}, keywords = {agn, enrichment, feedback, hydraa, icm}, month = {Sep}, posted-at = {2009-09-15 23:47:14}, priority = {2}, title = {Direct Evidence for Outflow of Metal-enriched Gas Along the Radio Jets of Hydra A}, url = {http://arxiv.org/abs/0909.2252}, year = {2009} }

TY - JOUR ID - citeulike:5785379 L3 - citeulike-article-id:5785379 N2 - Using deep Chandra observations of the Hydra A galaxy cluster, we examine the metallicity structure near the central galaxy and along its powerful radio source. We show that the metallicity of the intracluster medium is enhanced by up to 0.2 dex along the radio jets and lobes compared to the metallicity of the undisturbed gas. The enhancements extend from a radius of 20 kpc from the central galaxy to a distance of ~ 120 kpc. We estimate the total iron mass that has been transported out of the central galaxy to be between 2 x 10^7 M_sun and 7 x 10^7 M_sun which represents 10% - 20% of the iron mass within the central galaxy. The energy required to lift this gas is roughly 1% to 5% of the total energetic output of the AGN. Evidently, Hydra A's powerful radio source is able to redistribute metal-enriched, low entropy gas throughout the core of the galaxy cluster. The short re-enrichment time scale < 10^9 yr implies that the metals lost from the central galaxy will be quickly replenished. TI - Direct Evidence for Outflow of Metal-enriched Gas Along the Radio Jets of Hydra A KW - agn KW - enrichment KW - feedback KW - hydraa KW - icm AU - Kirkpatrick, CC AU - Gitti, M AU - Cavagnolo, KW AU - McNamara, BR AU - David, LP AU - Nulsen, PEJ AU - Wise, MW PY - 2009/Sep/11/ UR - http://arxiv.org/abs/0909.2252 ER -