Do Massive Primordial Disks Evolve Into Massive Debris Disks?

Astronomy and Astrophysics – Astronomy

Scientific paper

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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.

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