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@ARTICLE{Pfalzner:911746,
      author       = {Pfalzner, Susanne and Dehghani, Shahrzad and Michel,
                      Arnaud},
      title        = {{M}ost {P}lanets {M}ight {H}ave {M}ore than 5 {M}yr of
                      {T}ime to {F}orm},
      journal      = {The astrophysical journal / 2},
      volume       = {939},
      number       = {1},
      issn         = {2041-8205},
      address      = {London},
      publisher    = {Institute of Physics Publ.},
      reportid     = {FZJ-2022-04998},
      pages        = {L10 -},
      year         = {2022},
      abstract     = {The lifetime of protoplanetary disks is a crucial parameter
                      for planet formation research. Observations of disk
                      fractions in star clusters imply median disk lifetimes of
                      1–3 Myr. This very short disk lifetime calls for planet
                      formation to occur extremely rapidly. We show that young,
                      distant clusters (≤5 Myr, >200 pc) often dominate these
                      types of studies. Such clusters frequently suffer from
                      limiting magnitudes leading to an over-representation of
                      high-mass stars. As high-mass stars disperse their disks
                      earlier, the derived disk lifetimes apply best to high-mass
                      stars rather than low-mass stars. Including only nearby
                      clusters (<200 pc) minimizes the effect of limiting
                      magnitude. In this case, the median disk lifetime of
                      low-mass stars is with 5–10 Myr, thus much longer than
                      often claimed. The longer timescales provide planets ample
                      time to form. How high-mass stars form planets so much
                      faster than low-mass stars is the next grand challenges.},
      cin          = {JSC},
      ddc          = {520},
      cid          = {I:(DE-Juel1)JSC-20090406},
      pnm          = {5111 - Domain-Specific Simulation $\&$ Data Life Cycle Labs
                      (SDLs) and Research Groups (POF4-511)},
      pid          = {G:(DE-HGF)POF4-5111},
      typ          = {PUB:(DE-HGF)16},
      UT           = {WOS:000874338400001},
      doi          = {10.3847/2041-8213/ac9839},
      url          = {https://juser.fz-juelich.de/record/911746},
}