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Star Formation Studies with the Sloan Digital Sky Survey.


PB2001105826

Publication Date 2001
Personal Author McGehee, P. M.
Page Count 4
Abstract The determination of timescales associated with planetary formation and circumstellar disk evolution requires large samples of stars having diverse environments and ages. Such a sample can be obtained using the Sloan Digital Sky Survey as it is systematically mapping one-quarter of the entire sky providing photometric data on over 100 million objects in five passbands.
Keywords
  • Star formation
  • Planetary formation
  • Star distribution
  • Stars
  • Spectroscopy
  • Photometry
  • Mapping
  • Planetary evolution
  • Passbands
  • Sky surveys(Astronomy)
Source Agency
  • Technical Information Center Oak Ridge Tennessee
NTIS Subject Category
  • 54C - Astrophysics
Corporate Authors Los Alamos National Lab., NM.; Department of Energy, Washington, DC.
Supplemental Notes Sponsored by Department of Energy, Washington, DC.
Document Type Technical Report
NTIS Issue Number 200117
Contract Number
  • DE-W-7405-ENG-36
Star Formation Studies with the Sloan Digital Sky Survey.
Star Formation Studies with the Sloan Digital Sky Survey.
PB2001105826

  • Star formation
  • Planetary formation
  • Star distribution
  • Stars
  • Spectroscopy
  • Photometry
  • Mapping
  • Planetary evolution
  • Passbands
  • Sky surveys(Astronomy)
  • Technical Information Center Oak Ridge Tennessee
  • 54C - Astrophysics
  • DE-W-7405-ENG-36
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