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Assembly bias evidence in close galaxy pairs

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اقرأ أكثر حفظ في قائمتي
  • معلومة اضافية
    • بيانات النشر:
      Oxford University Press (OUP)
    • الموضوع:
      2019
    • Collection:
      University of Central Lancashire: CLOK - Central Lancashire Online Knowledge
    • نبذة مختصرة :
      The growth channel of massive galaxies involving mergers can be studied via close pairs as putative merger progenitors, where the stellar populations of the satellite galaxies will be eventually incorporated into the massive primaries. We extend our recent analysis of the GAMA-based sample of close pairs presented in Ferreras et al. to the general spectroscopic dataset of SDSS galaxies (DR14), for which the high S/N of the data enables a detailed analysis of the differences between satellite galaxies with respect to the mass of the primary galaxy. A sample of approximately two thousand satellites of massive galaxies is carefully selected within a relatively narrow redshift range (0.07
    • File Description:
      application/pdf
    • Relation:
      https://clok.uclan.ac.uk/id/eprint/28600/1/28600%20stz1286.pdf; https://clok.uclan.ac.uk/id/eprint/28600/9/28600%20stz1286%20published.pdf; Ferreras, I, Hopkins, A M, Lagos, C, Sansom, Anne E orcid iconorcid:0000-0002-2782-7388 , Scott, N, Croom, S and Brough, S (2019) Assembly bias evidence in close galaxy pairs. Monthly Notices of the Royal Astronomical Society, 487 (1). pp. 435-443. ISSN 0035-8711
    • الرقم المعرف:
      10.1093/mnras/stz1286
    • الدخول الالكتروني :
      https://clok.uclan.ac.uk/id/eprint/28600/
      https://clok.uclan.ac.uk/id/eprint/28600/1/28600%20stz1286.pdf
      https://clok.uclan.ac.uk/id/eprint/28600/9/28600%20stz1286%20published.pdf
      https://doi.org/10.1093/mnras/stz1286
    • Rights:
      cc_by_nc_nd_4 ; cc_by_4
    • الرقم المعرف:
      edsbas.D18327F3