![](/images/ico/ico_close.png)
![](/images/ico/ico5.png)
Author: De Donder E. Vanbeveren D.
Publisher: Elsevier
ISSN: 1384-1076
Source: New Astronomy, Vol.8, Iss.5, 2003-07, pp. : 415-425
Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.
Abstract
Related content
![](/images/ico/ico_close.png)
![](/images/ico/ico5.png)
5. INITIAL MASS FUNCTIONS, STAR FORMATION RATES AND CHEMICAL EVOLUTION WITH z
Astrophysics and Space Science, Vol. 276, Iss. 2-4, 2001-01 ,pp. :
![](/images/ico/ico_close.png)
![](/images/ico/ico5.png)
![](/images/ico/ico_close.png)
![](/images/ico/ico5.png)
Chemical evolution in simulations of galaxy formation
By Portinari Laura Carraro Giovanni Lia Cesario
Astrophysics and Space Science, Vol. 281, Iss. 1-2, 2002-07 ,pp. :
![](/images/ico/ico_close.png)
![](/images/ico/ico5.png)
A model for the population of helium stars in the Galaxy: Low-mass stars
Astronomy Reports, Vol. 49, Iss. 11, 2005-11 ,pp. :