The Rotation Period Distribution of Pre-Main-Sequence Stars in and around the Orion Nebula

Details The Rotation Period Distribution of Pre-Main-Sequence Stars in and around the Orion Nebula The Rotation Period Distribution of Pre-Main-Sequence Stars in and around the Orion Nebula

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aj....117.2941s&link_type=abstract

The Astronomical Journal, Volume 117, Issue 6, pp. 2941-2979.

Astronomy and Astrophysics

Astronomy

183

Stars: Evolution, Stars: Pre-Main-Sequence, Stars: Rotation, Stars: Spots

Scientific paper

We report rotation periods for 254 stars in an area 40'x80' centered on the Orion Nebula. We show that these stars are likely members of the young (~10^6 yr) Orion OBIc/d association. The rotation period distribution we determine, which is sensitive to periods 0.1

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