Related content

The radio galaxy K-z relation: The $\mathsf{10^{12}}~$M$\mathsf{_\odot}$ mass limit

By  

Astronomy & Astrophysics, Vol. 415, Iss. 3, 2004-03 ,pp. : 931-940

Edp Sciences

Access to resources Recommend Favorite

Colour evolution of disk galaxy models from $\vec{z}=\mathsf{4}$ to $\vec{z}=\mathsf{0}$

By  

Astronomy & Astrophysics, Vol. 389, Iss. 3, 2002-07 ,pp. : 761-778

Edp Sciences

Access to resources Recommend Favorite

Simulating the mass-metallicity relation from z $\mathsf{\sim}$ 1

By  

Astronomy & Astrophysics, Vol. 486, Iss. 3, 2008-08 ,pp. : 711-720

Edp Sciences

Access to resources Recommend Favorite

A new deuterium abundance measurement from a damped Ly$\alpha$ system at $\vec{z}_{\mathsf{abs}} =\mathsf{3.025}$

By  

Astronomy & Astrophysics, Vol. 368, Iss. 3, 2001-03 ,pp. : L21-L24

Edp Sciences

Access to resources Recommend Favorite

VLT adaptive optics imaging of QSO host galaxies and their close environment at z $\mathsf{\sim}$ 2.5: Results from a pilot program

By  

Astronomy & Astrophysics, Vol. 434, Iss. 2, 2005-05 ,pp. : 469-473

Edp Sciences

Access to resources Recommend Favorite