Quantifying the suppression of the (un)-obscured star formation in galaxy cluster cores at 0.2 less than or similar to z less than or similar to 0.9

Research output: Contribution to journal › Journal article › Research › peer-review

Documents

  • sty3335

    Final published version, 3.62 MB, PDF document

  • L. Rodriguez-Munoz
  • G. Rodighiero
  • C. Mancini
  • P. G. Perez-Gonzalez
  • T. D. Rawle
  • E. Egami
  • A. Mercurio
  • P. Rosati
  • A. Puglisi
  • A. Franceschini
  • I. Balestra
  • I. Baronchelli
  • A. Biviano
  • H. Ebeling
  • A. C. Edge
  • A. F. M. Enia
  • C. Grillo
  • C. P. Haines
  • E. Iani
  • T. Jones
  • And 4 others
  • M. Nonino
  • I. Valtchanov
  • B. Vulcani
  • M. Zemcov
Original languageEnglish
JournalMonthly Notices of the Royal Astronomical Society
Volume485
Issue number1
Pages (from-to)586-619
Number of pages34
ISSN0035-8711
DOIs
Publication statusPublished - 1 May 2019

    Research areas

  • galaxies: clusters: general, galaxies: evolution, galaxies: star formation, catalogues

Links

ID: 234880036