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・ RWTH Aachen University
・ RWTH ASR
・ RWTH FSA Toolkit
・ RWU
・ Rx
・ Rx (band)
・ RX (rocket family)
・ RX Andromedae
・ Rx Bandits
・ RX II
・ RX J0720.4-3125
・ RX J0806.3+1527
・ RX J0822-4300
・ RX J0852.0-4622
・ RX J1131-1231
RX J1347.5-1145
・ RX J1416.5+2315
・ RX J1856.5-3754
・ RX Leporis
・ RX meter
・ RX microcontroller family
・ RX Soori
・ RX Telescopii
・ RX-250-LPN
・ RX2
・ RX5
・ RXJ1242-11
・ RxList
・ RXNO Ontology
・ RxNorm


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RX J1347.5-1145 : ウィキペディア英語版
RX J1347.5-1145

RX J1347.5–1145 is one of the most X-ray-luminous and most massive galaxy clusters known.〔(Dark Matter and Baryons in the X-Ray Luminous Merging Galaxy Cluster RX J1347.5–1145 )〕 Redshift was noted as z=0.451 with an X-ray luminosity of 1045 ergs s−1 in a paper from 2002.〔(S. Ravindranath and L. C. Ho - Magellan Spectroscopy of the Galaxy Cluster RX J1347.5-1145: Redshift Estimates for the Gravitationally Lensed Arcs (2002) )〕 In 2013, one study found eight cases of the same object resulting from the intense gravitational bending of light.〔(F. Köhlinger and R.W. Schmidt - Strong lensing in RX J1347.5-1145 revisited (2013) )〕 That study made use of data from Cluster Lensing And Supernova survey with Hubble (CLASH) as well as other sources.〔 The cluster is roughly 5 billion light years away from our Solar System.
==References==


抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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