First EUV search for He I lines from a z=0.7 cool-core cluster yields non-detections and upper limits on 3e4 K gas, but the limits are too weak to rule out the steady cooling flow.
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The first astrophysical result of HISAKI: a search for the EUV He I lines a massive cool core cluster at z=0.7
First EUV search for He I lines from a z=0.7 cool-core cluster yields non-detections and upper limits on 3e4 K gas, but the limits are too weak to rule out the steady cooling flow.