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2005MNRAS.358..341L - Mon. Not. R. Astron. Soc., 358, 341-352 (2005/April-1)
Do accretion discs regulate the rotation of young stars?
LITTLEFAIR S.P., NAYLOR T., BURNINGHAM B. and JEFFRIES R.D.
Abstract (from CDS):
We also present a discussion of our own IC 348 data in the context of previously published period distributions for the ONC, the Orion flanking fields and NGC 2264. We find that the previously claimed correlation between infrared excess and rotation period in the ONC might, in fact, result from a correlation between infrared excess and mass. We also find a marked difference in period distributions between NGC 2264 and IC 348, which presents a serious challenge to the disc-locking paradigm, given the similarity in ages and disc fractions between the two clusters.
Abstract Copyright: 2005 RAS
Journal keyword(s): accretion, accretion discs - planetary systems: protoplanetary discs - stars: pre-main-sequence
VizieR on-line data: <Available at CDS (J/MNRAS/358/341): ic348.dat table1.dat>
Nomenclature: Table 1: Cl* IC 348 LNB NNN N=292 among (Nos 1-342).
CDS comments: KH 15D = Cl* NGC 2264 VVO 15D.
Simbad objects: 297
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