SIMBAD references

2006ApJ...646..297R - Astrophys. J., 646, 297-303 (2006/July-3)

A correlation between Pre-Main-Sequence stellar rotation rates and IRAC excesses in Orion.

REBULL L.M., STAUFFER J.R., MEGEATH S.T., HORA J.L. and HARTMANN L.

Abstract (from CDS):

Early observations of T Tauri stars suggested that stars with evidence of circumstellar accretion disks rotated slower than stars without such evidence, but more recent results are not as clear. Near-IR circumstellar disk indicators, although the most widely available, are subject to uncertainties that can result from inner disk holes and/or the system inclination. Mid-infrared observations are less sensitive to such effects, but until now, these observations have been difficult to obtain. The Spitzer Space Telescope now easily enables mid-infrared measurements of large samples of PMS stars covering a broad mass range in nearby star-forming regions. Megeath and collaborators surveyed the Orion Molecular Clouds (∼1 Myr) with the IRAC instrument (3.6, 4.5, 5.8, 8 µm) as part of a joint IRAC and MIPS GTO program. We examine the relationship between rotation and Spitzer mid-IR fluxes for ∼900 stars in Orion for stars between 3 and 0.1 M. We find in these Spitzer data the clearest indication to date that stars with longer periods are more likely than those with short periods to have IR excesses suggestive of disks.

Abstract Copyright:

Journal keyword(s): Galaxy: Open Clusters and Associations: Individual: Name: Orion - Stars: Rotation

VizieR on-line data: <Available at CDS (J/ApJ/646/297): table1.dat>

Status at CDS:  

Simbad objects: 471

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2006ApJ...646..297R and select 'bookmark this link' or equivalent in the popup menu


2020.03.28-13:47:25

© Université de Strasbourg/CNRS

    • Contact