光侵蝕

這種侵蝕阻礙了環繞著原恆星中心核的外圍吸積，因此，反過來也阻止了原恆星成為成熟的恆星，使得原恆星只能發展成為棕矮星或行星質量天體[1]。

光侵蝕是星前核心因為附近恆星的電離輻射導致外層的色散。

參考資料
  1. The formation of free-floating brown dwarves and planetary-mass objects by photo-erosion of prestellar cores, A. P. Whitworth, H. Zinnecker, Astronomy & Astrophysics, Volume 427, Number 1, November III 2004, Page(s) 299 - 306, doi:10.1051/0004-6361:20041131


This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.