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Home All issues A&A, 383 1 (2002) 210-217 Article references

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Cited article:

The active lives of stars: A complete description of the rotation and XUV evolution of F, G, K, and M dwarfs

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Astronomy & Astrophysics 649 A96 (2021)
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The Relative Emission from Chromospheres and Coronae: Dependence on Spectral Type and Age*

Jeffrey L. Linsky, Brian E. Wood, Allison Youngblood, Alexander Brown, Cynthia S. Froning, Kevin France, Andrea P. Buccino, Steven R. Cranmer, Pablo Mauas, Yamila Miguel, J. Sebastian Pineda, Sarah Rugheimer, Mariela Vieytes, Peter J. Wheatley and David J. Wilson
The Astrophysical Journal 902 (1) 3 (2020)
https://doi.org/10.3847/1538-4357/abb36f

Stars with solar-type activity: GTSh10 catalogue

R. E. Gershberg, A. V. Terebizh and A. A. Shlyapnikov
Bulletin of the Crimean Astrophysical Observatory 107 (1) 11 (2011)
https://doi.org/10.3103/S0190271711010062

X-RAY VARIABILITY OF σ ORIONIS YOUNG STARS AS OBSERVED WITHROSAT

J. A. Caballero, J. López-Santiago, E. de Castro and M. Cornide
The Astronomical Journal 137 (6) 5012 (2009)
https://doi.org/10.1088/0004-6256/137/6/5012

Recent X-ray studies of stellar cycles and long-term variability

Giovanni Peres, Giuseppina Micela and Fabio Favata
Proceedings of the International Astronomical Union 2 (14) (2006)
https://doi.org/10.1017/S1743921307010630

A Comparative Study of Flaring Loops in Active Stars

D. J. Mullan, M. Mathioudakis, D. S. Bloomfield and D. J. Christian
The Astrophysical Journal Supplement Series 164 (1) 173 (2006)
https://doi.org/10.1086/502629

NEXXUS: A comprehensive ROSAT survey of coronal X-ray emission among nearby solar-like stars

J. H. M. M. Schmitt and C. Liefke
Astronomy & Astrophysics 417 (2) 651 (2004)
https://doi.org/10.1051/0004-6361:20030495

High-amplitude, long-term X-ray variability in the solar-type star HD 81809: The beginning of an X-ray activity cycle?

F. Favata, G. Micela, S. L. Baliunas, et al.
Astronomy & Astrophysics 418 (1) L13 (2004)
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Coronal Variability in the Young Cluster NGC 2516

S. J. Wolk, F. R. Harnden, Jr., S. S. Murray, et al.
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Are Coronae of Late‐Type Stars Made of Solar‐like Structures? The X‐Ray Surface Flux versus Hardness Ratio Diagram and the Pressure‐Temperature Correlation

G. Peres, S. Orlando and F. Reale
The Astrophysical Journal 612 (1) 472 (2004)
https://doi.org/10.1086/422461

X-ray variability of Pleiades late-type stars as observed with the ROSAT-PSPC

A. Marino, G. Micela, G. Peres and S. Sciortino
Astronomy & Astrophysics 406 (2) 629 (2003)
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Dependence of coronal X-ray emission on spot-induced brightness variations in cool main sequence stars

S. Messina, N. Pizzolato, E. F. Guinan and M. Rodonò
Astronomy & Astrophysics 410 (2) 671 (2003)
https://doi.org/10.1051/0004-6361:20031203

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

N. Pizzolato, A. Maggio, G. Micela, S. Sciortino and P. Ventura
Astronomy & Astrophysics 397 (1) 147 (2003)
https://doi.org/10.1051/0004-6361:20021560