The stellar activity-rotation relationship revisited: Dependence of saturated and non-saturated X-ray emission regimes on stellar mass for late-type dwarfs-Reference-Cited by-同舟云学术

The stellar activity-rotation relationship revisited: Dependence of saturated and non-saturated X-ray emission regimes on stellar mass for late-type dwarfs

Published:2002-12-11 Issue:1 Volume:397 Page:147-157
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Pizzolato N.,Maggio A.,Micela G.,Sciortino S.,Ventura P.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:20021560/pdf

Reference62 articles.

1. Rotation Periods of Late‐Type Stars in the Young Open Cluster IC 2602

2. Periodic low-amplitude variations in the brightness of Proxima Centauri

3. VRI photometry - an addendum

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