Inferring rotation periods of young stars from synoptic observations

Patrick Hartigan, Christopher M. Johns-Krull, Paul Scowen

Research output: Chapter in Book/Report/Conference proceedingChapter

Abstract

Using known distributions for the periods, amplitudes and light-curve shapes of young stars, we examine how well one could measure periods of these objects in the upcoming era of large synoptic surveys. Surveys like the LSST should be able to recover accurate rotation periods for over 90% of targets of interest in regions near to massive-star formation. That information will usher in a new era in our understanding of how the angular momentum of a young star/disk system evolves with time.

Original languageEnglish (US)
Title of host publicationNew Horizons in Time-Domain Astronomy
EditorsElizabeth Griffin, Robert J. Hanisch, Robert L. Seaman
Pages327-330
Number of pages4
EditionS285
DOIs
StatePublished - Sep 1 2011

Publication series

NameProceedings of the International Astronomical Union
NumberS285
Volume7
ISSN (Print)1743-9213
ISSN (Electronic)1743-9221

Keywords

  • stars: pre-main-sequence
  • stars: rotation

ASJC Scopus subject areas

  • Medicine (miscellaneous)
  • Astronomy and Astrophysics
  • Nutrition and Dietetics
  • Public Health, Environmental and Occupational Health
  • Space and Planetary Science

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