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A Search for Disk-Locking in the Chamaeleon I Star Forming Region
Stockholm University, Faculty of Science, Department of Astronomy.
2008 (English)In: Precision Spectroscopy in Astrophysics, 2008Conference paper, Published paper (Other academic)
Abstract [en]

We investigated the connection between disks and stellar rotation. Disk-locking theory predicts that accreting stars are preferentially slow rotators compared to their peers. If true, classical T Tauri stars (CTTS), which are accreting based on strong Hα, emission, should have observably lower vsini, values compared to weak-lined T Tauri stars (WTTS), which are not accreting. We present our findings from high-resolution optical spectra taken with the Magellan Inamori Kyocera Echelle (MIKE) spectrograph on the Magellan Clay 6.5-m telescope located at the Las Campanas Observatory of 63 T Tauri stars in the Cha I SFR.

Place, publisher, year, edition, pages
2008.
Identifiers
URN: urn:nbn:se:su:diva-15372OAI: oai:DiVA.org:su-15372DiVA: diva2:181892
Note
Precision Spectroscopy in Astrophysics, Proceedings of the ESO/Lisbon/Aveiro Conference held in Aveiro, Portugal, 11-15 September 2006. Edited by N.C. Santos, L. Pasquini, A.C.M. Correia, and M. Romanielleo. Garching, Germany, 2008 pp. 307-308Available from: 2008-12-01 Created: 2008-12-01Bibliographically approved

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http://adsabs.harvard.edu/abs/2008psa..conf..307N

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