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  • 标题:Erratum: “Spiral Arms in Disks: Planets or Gravitational Instability?” (2018, ApJ, 862, 103)
  • 本地全文:下载
  • 作者:Ruobing Dong ; Joan R.Najita ; Sean Brittain
  • 期刊名称:The Astronomical journal
  • 印刷版ISSN:0004-6256
  • 电子版ISSN:1538-3881
  • 出版年度:2021
  • 卷号:163
  • 期号:1
  • 页码:1-1
  • DOI:10.3847/1538-3881/ac3418
  • 语种:English
  • 出版社:American Institute of Physics
  • 摘要:This Erratum is to clarify a potential confusion regarding Equation (2) in the Appendix B in Dong et al. (2018). The factor of 0.5 in 0.5 Rmm is an approximate correction factor meant to identify the radius where the dust temperature is the global average in a disk whose size is Rmm. This is to account for the fact that dust at different radii has different temperature. If the surface density follows a Σ ∼ 1/R radial profile and the disk extends from R = 0 to R = Rmm, 0.5 Rmm is the half-mass radius, i.e., the radius inside which half of the disk mass is enclosed. Equation (2) in the Appendix B is a fit to simulations to give the specific temperature at R = 0.5Rmm, not Rmm, in a disk; this temperature is considered as a proxy for the average dust temperature in a disk whose outer edge is at Rmm.
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