CL J1001 + 0220

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CL J1001 with the superimposed images from the Chandra telescope , from the Atacama Large Millimeter Array and the Ultra VISTA

CL J1001 + 0220 or CL J1001 for short is a galaxy cluster in the constellation Sextant with a redshift of . The cluster was discovered in 2016 with the help of the Chandra Telescope , the Atacama Large Millimeter Array and the VISTA . The galaxy cluster consists of 17 members, 13 of which form the core of CL J10001, which is approximately 80,000 pc in diameter . The core of the cluster has an infrared luminosity of 10 13.2 the luminosity of the sun and this results in a star formation rate of 3400 solar masses per year. The gas required for star formation will be exhausted in around 200 million years.

Members

Surname Right ascension declination Spectral redshift Mass (in solar mass) Remarks
ID 128484 150.22348 2.30719 2,495 10 10.82
ID 129305 150.23940 2.31750 2.512 10 10.19
ID 129444 150.24875 2.31921 2.510 10 10.77
ID 131661 150.23584 2.34488 2.501 10 11.03
ID 131864 150.23454 2,34770 2.511 10 10.38
ID 132636 150.22505 2.35620 2.510 10 10.68
ID 130359 150.22899 2,32978 2.507 10 11.26
ID 130842 150.23746 2,33612 2.515 10 11.12
ID 130891 150.23987 2,33645 2.513 10 11.06
ID 130901 150.23923 2,33637 2.508 10 11.58
ID 130933 150.23869 2,33683 2.504 10 11.29 Active galaxy core
ID 130949 150.23701 2.33571 2.503 10 11.57
ID 131077 150.23735 2,33814 2,494 10 11.16
ID 131079 150.23695 2,33748 2.502 10 11.36
ID 132044 150.23650 2,34881 2.504 10 11.13
ID 132627 150.23421 2.35659 2.506 10 10.90
not named 150.23419 2,33647 2.504 10 11.0

Individual evidence

  1. ↑ Tao Wang, David Elbaz, Emanuele Daddi, Alexis Finoguenov, Daizhong Liu, Corenin Schrieber, Sergio Martin, Veronica Strazzullo, Francesco Valentino, Remco van Der Burg, Anita Zanella, Laure Cisela, Raphael Gobat, Amandine Le Brun, Maurilio Pannella, Mark Sargent, Xinwen Shu, Qinghua Tan, Nico Cappelluti, Xanxia Li: Discovery of a galaxy cluster with a violently starbursting core at z = 2.506 . In: The Astrophysical Journal . 828, 2016. arxiv : 1604.07404 . doi : 10.3847 / 0004-637X / 828/1/56 .