The self-enrichment of galactic halo globular cluster: a clue to their formation ?

Table 1.


Dependence of [Fe/H] on Ph

Ph[dyne.cm-2] log10Mc/ [Fe/H]
10-9
10-10
10-11		 5.5
6.0
6.5 		-1.2
-1.7
-2.2


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