X-Ray Properties of Pre-Main-Sequence Stars in the Orion Nebula Cluster with Known Rotation Periods

Author:

Stassun Keivan G.,Ardila David R.,Barsony Mary,Basri Gibor,Mathieu Robert D.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference41 articles.

1. Alencar, S. H. P. & Batalha, C. 2001, in ASP Conf. Ser. 244, Young Stars Near Earth: Progress and Prospects, ed. R. Jayawardhana & T. P. Greene (San Francisco: ASP), 141

2. Ardila, D. R., etal 2004, in Open Issues in Local Star Formation, ed. J. R. D. Lepine & J. C. Gregorio-Hetem (Dordrecht: Kluwer), in press

3. Arnaud, K. A. 1996, in ASP Conf. Ser. 101, Astronomical Data Analysis Software and Systems V, ed. G. H. Jacoby & J. Barnes (San Francisco: ASP), 17

4. On the Rotational Evolution of Solar‐ and Late‐Type Stars, Its Magnetic Origins, and the Possibility of Stellar Gyrochronology

5. A Connection between the Morphology of the X-Ray Emission and Rotation for Solar-Type Stars in Open Clusters

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