Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21542815s&link_type=abstract
American Astronomical Society, AAS Meeting #215, #428.15; Bulletin of the American Astronomical Society, Vol. 42, p.347
Astronomy and Astrophysics
Astronomy
Scientific paper
Recent Spitzer IRAC observations of young stars in Orion and NGC 2264 have shown a strong link between primordial circumstellar disks and stellar rotation. Slow rotators show a larger percentage of stars with excess infrared emission than fast rotators. If stars with massive primordial disks evolve into massive debris disks, then massive debris disks should be more frequent among slow rotators. We present new MIPS 24um data for a large sample of post-accretion phase young stars in the Lower Centaurus Crux (LCC) area of the ScoCen region. A fully automated spectral energy distribution (SED) is used to identify small disk excesses in the observed young stars. By investigating the vsini measurements of stars that show infrared excess from this sample, we investigate if a link exists between rotation speeds and debris disks.
Bessell Michael
Rebull Luisa
Schneider Andreas
Song Inseok
Stauffer John
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