Implications of a non-universal IMF from C, N, and O abundances in very metal-poor Galactic stars and damped Lyα absorbers

Author： Tsujimoto T.   Bekki K.  

Publisher： Edp Sciences

E-ISSN： 1432-0746|530|issue|A78-A78

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.530, Iss.issue, 2011-05, pp. : A78-A78

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

Abstract

Related content

First stars VI – Abundances of C, N, O, Li, and mixing in extremely metal-poor giants. Galactic evolution of the light elements

By  

Astronomy & Astrophysics, Vol. 430, Iss. 2, 2005-02 ,pp. : 655-668

Edp Sciences

Access to resources Recommend Favorite

The emergence of the galactic stellar mass function from a non-universal IMF in clusters

By Dib Sami   Basu Shantanu  

Astronomy & Astrophysics, Vol. 614, Iss. issue, 2018-06 ,pp. : A43-A43

Edp Sciences

Access to resources Recommend Favorite

Mg abundances in metal-poor halo stars as a tracer of early Galactic mixing

By  

Astronomy & Astrophysics, Vol. 430, Iss. 2, 2005-02 ,pp. : 507-522

Edp Sciences

Access to resources Recommend Favorite

Sulphur and zinc abundances in Galactic stars and damped Ly$\alpha$ systems

By  

Astronomy & Astrophysics, Vol. 415, Iss. 3, 2004-03 ,pp. : 993-1007

Edp Sciences

Access to resources Recommend Favorite

Implications of O and Mg abundances in metal-poor halo stars for stellar iron yields

By  

Astronomy & Astrophysics, Vol. 388, Iss. 3, 2002-06 ,pp. : 842-860

Edp Sciences

Access to resources Recommend Favorite