DID FOMALHAUT, HR 8799, AND HL TAURI FORM PLANETS VIA THE GRAVITATIONAL INSTABILITY? PLACING LIMITS ON THE REQUIRED DISK MASSES Article (Web of Science)

cited authors

  • Nero, D.; Bjorkman, J. E.

publication date

  • September 10, 2009

webpage

published in

author keyword

  • instabilities
  • planetary systems: formation
  • planetary systems: protoplanetary disks
  • stars: individual (Fomalhaut, HL Tau, HR 8799)

category

start page

  • L163

end page

  • L167

volume

  • 702

issue

  • 2