Non-LTE line formation for heavy elements in four very metal-poor stars

E-ISSN： 1432-0746|478|2|529-541

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.478, Iss.2, 2008-02, pp. : 529-541

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

Non-LTE line formation for Pr ii and Pr iii in A and Ap stars

Astronomy & Astrophysics, Vol. 495, Iss. 1, 2009-02 ,pp. : 297-311

Edp Sciences

Access to resources Recommend Favorite

The non-LTE line formation of neutral carbon in late-type stars

Astronomy & Astrophysics, Vol. 458, Iss. 3, 2006-11 ,pp. : 899-914

Edp Sciences

Access to resources Recommend Favorite

Non-LTE Line Formation in the Near-IR: Hot Stars

EAS Publications Series, Vol. 43, Iss. issue, 2010-11 ,pp. : 199-214

Edp Sciences

Access to resources Recommend Favorite

Multi-level 3D non-LTE computations of lithium lines in the metal-poor halo stars HD 140283 and HD 84937

Astronomy & Astrophysics, Vol. 399, Iss. 3, 2003-03 ,pp. : L31-L34

Edp Sciences

Access to resources Recommend Favorite

Non-LTE abundances of Mg and K inextremely metal-poor stars and the evolution of [O/Mg], [Na/Mg], [Al/Mg], and [K/Mg] in the Milky Way*

By Andrievsky S. M. Spite M. Korotin S. A. Spite F. Bonifacio P. Cayrel R. François P. Hill V.

Astronomy & Astrophysics, Vol. 509, Iss. issue, 2010-01 ,pp. : A88-A88

Edp Sciences

Access to resources Recommend Favorite