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@ARTICLE{Zhu:1020571,
      author       = {Zhu, Qirong and Pérez-Montaño, Luis Enrique and
                      Rodriguez-Gomez, Vicente and Cervantes Sodi, Bernardo and
                      Zjupa, Jolanta and Marinacci, Federico and Vogelsberger,
                      Mark and Hernquist, Lars},
      title        = {{G}iant low surface brightness galaxies in {TNG}100},
      journal      = {Monthly notices of the Royal Astronomical Society},
      volume       = {523},
      number       = {3},
      issn         = {0035-8711},
      address      = {Oxford},
      publisher    = {Oxford Univ. Press},
      reportid     = {FZJ-2024-00266},
      pages        = {3991 - 4014},
      year         = {2023},
      abstract     = {Giant low surface brightness (GLSB) galaxies, such as Malin
                      1 and UGC 1382, contain the largest stellar discs known.
                      GLSB galaxies also often contain large masses of neutral
                      hydrogen (H I). However, these extreme galaxies' origin and
                      properties remain poorly understood. Using the cosmological
                      simulation IllustrisTNG 100, we identify and select a sample
                      of ~200 galaxies with extended (RHI>50 kpc) and well-defined
                      H I discs, ~6 per cent of the total galaxies in the same
                      stellar mass range (10.2 < log (M*/M⊙) < 11.6). This GLSB
                      sample is heterogeneous, with mixed galaxy morphologies
                      ranging from the most disc-dominated systems to massive
                      ellipticals. These simulated GLSB galaxies are located in
                      massive haloes (Vmax>150 km s−1) and their properties,
                      such as total H I content, stellar disc parameters, star
                      formation rate, and rotation curves, agree with observed
                      GLSB galaxies. We construct a paired control sample to
                      contrast with the GLSB galaxies. The GLSB galaxies tend to
                      have large galaxy spin parameters (40 per cent larger) and
                      larger ex situ stellar mass fractions than the paired
                      control. We find evidence that aligned mergers promote the
                      formation of extended discs and that isolated environments
                      help the survival of those discs across cosmic time.},
      cin          = {JSC},
      ddc          = {520},
      cid          = {I:(DE-Juel1)JSC-20090406},
      pnm          = {5112 - Cross-Domain Algorithms, Tools, Methods Labs (ATMLs)
                      and Research Groups (POF4-511) / DFG project 15499703 - TRR
                      33: Das Dunkle Universum (15499703) / ATMLAO - ATML
                      Application Optimization and User Service Tools (ATMLAO)},
      pid          = {G:(DE-HGF)POF4-5112 / G:(GEPRIS)15499703 /
                      G:(DE-Juel-1)ATMLAO},
      typ          = {PUB:(DE-HGF)16},
      UT           = {WOS:001011067600017},
      doi          = {10.1093/mnras/stad1655},
      url          = {https://juser.fz-juelich.de/record/1020571},
}