Subphotospheric convection and magnetic activity dependence on metallicity and age: Models and tests
A&A, 373 2 (2001) 597-607
Published online: 2001-07-15
Articles citing this article
The Citing articles tool gives a list of articles citing the current article.
The citing articles come from EDP Sciences database, as well as other publishers participating in CrossRef Cited-by Linking Program. You can set up your personal account to receive an email alert each time this article is cited by a new article (see the menu on the right-hand side of the abstract page).
Cited article:
This article has been cited by the following article(s):
Dispersal timescale of protoplanetary disks in the low-metallicity young cluster Dolidze 25
M. G. Guarcello, K. Biazzo, J. J. Drake, et al.Astronomy & Astrophysics 650 A157 (2021)
https://doi.org/10.1051/0004-6361/202140361
Rossby number and chromospheric activity of solar mass stars
Philippe GondoinAstronomische Nachrichten 341 (5) 557 (2020)
https://doi.org/10.1002/asna.202013723
X-ray emission regimes and rotation sequences in M 35
P. GondoinAstronomy & Astrophysics 556 A14 (2013)
https://doi.org/10.1051/0004-6361/201321076
DISCOVERY OF X-RAY EMISSION FROM YOUNG SUNS IN THE SMALL MAGELLANIC CLOUD
L. M. Oskinova, W. Sun, C. J. Evans, et al.The Astrophysical Journal 765 (1) 73 (2013)
https://doi.org/10.1088/0004-637X/765/1/73
Solar Activity and Deep Convection Modeling
O. V. Arkhypov, O. V. Antonov and M. L. KhodachenkoSolar Physics 282 (1) 39 (2013)
https://doi.org/10.1007/s11207-012-0139-x
Star formation in the outer Galaxy: coronal properties of NGC 1893
M. Caramazza, G. Micela, L. Prisinzano, et al.Astronomy & Astrophysics 539 A74 (2012)
https://doi.org/10.1051/0004-6361/201117256
Dynamo regime transition among Sun-like stars in M 34
P. GondoinAstronomy & Astrophysics 546 A117 (2012)
https://doi.org/10.1051/0004-6361/201219823
TESTING A PREDICTIVE THEORETICAL MODEL FOR THE MASS LOSS RATES OF COOL STARS
Steven R. Cranmer and Steven H. SaarThe Astrophysical Journal 741 (1) 54 (2011)
https://doi.org/10.1088/0004-637X/741/1/54
Theoretical values of convective turnover times and Rossby numbers for solar-like, pre-main sequence stars
N. R. Landin, L. T. S. Mendes and L. P. R. VazAstronomy and Astrophysics 510 A46 (2010)
https://doi.org/10.1051/0004-6361/200913015
XMM-Newton observations of the young open cluster Blanco 1
I. Pillitteri, G. Micela, S. Sciortino, F. Damiani and F. R. HarndenAstronomy & Astrophysics 421 (1) 175 (2004)
https://doi.org/10.1051/0004-6361:20035869
The X-ray Luminosity Distributions of the high-metallicity open cluster Blanco 1
I. Pillitteri, G. Micela, S. Sciortino and F. FavataAstronomy & Astrophysics 399 (3) 919 (2003)
https://doi.org/10.1051/0004-6361:20021818
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. VenturaAstronomy & Astrophysics 397 (1) 147 (2003)
https://doi.org/10.1051/0004-6361:20021560
From the Heart of the Ghoul: C and N Abundances in the Corona of Algol B
Jeremy J. DrakeThe Astrophysical Journal 594 (1) 496 (2003)
https://doi.org/10.1086/375837
Is Praesepe really different from the coeval Hyades cluster? The XMM-Newton view
E. Franciosini, S. Randich and R. PallaviciniAstronomy & Astrophysics 405 (2) 551 (2003)
https://doi.org/10.1051/0004-6361:20030623