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

Publisher： Edp Sciences

E-ISSN： 1432-0746|397|1|147-157

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.397, Iss.1, 2003-01, pp. : 147-157

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Related content

Dependence of the low-mass X-ray binary population on stellar age

By Zhang Z.   Gilfanov M.   Bogdán Á.  

Astronomy & Astrophysics, Vol. 546, Iss. issue, 2012-10 ,pp. : A36-A36

Edp Sciences

Access to resources Recommend Favorite

The onset of X-ray emission in young stellar objects

By  

Astronomy & Astrophysics, Vol. 463, Iss. 1, 2007-02 ,pp. : 275-288

Edp Sciences

Access to resources Recommend Favorite

The X-ray activity-rotation relation of T Tauri stars in Taurus-Auriga

By  

Astronomy & Astrophysics, Vol. 468, Iss. 2, 2007-06 ,pp. : 413-424

Edp Sciences

Access to resources Recommend Favorite

High mass X-ray binaries in the LMC: Dependence on the stellar population age and the “propeller” effect

By  

Astronomy & Astrophysics, Vol. 431, Iss. 2, 2005-02 ,pp. : 597-614

Edp Sciences

Access to resources Recommend Favorite

Mg line formation in late-type stellar atmospheres

By Osorio Y.   Barklem P. S.   Lind K.   Belyaev A. K.   Spielfiedel A.   Guitou M.   Feautrier N.  

Astronomy & Astrophysics, Vol. 579, Iss. issue, 2015-06 ,pp. : A53-A53

Edp Sciences

Access to resources Recommend Favorite