On the determination of the He abundance distribution in globular clusters from the width of the main sequence
One crucial piece of information to study the origin of multiple stellar populations in globular clusters is the range of initial helium abundances ΔY amongst the sub-populations hosted by each cluster. These estimates are commonly obtained by measuring the width in colour of the unevolved main sequence in an optical colour-magnitude diagram (CMD)
Cassisi, S. et al.
Fecha de publicación:
1
2017