  We investigate the Hagedorn transitions of string networks with Y-junctions
as may occur, for example, with (p,q) cosmic superstrings. In a simplified
model with three different types of string, the partition function reduces to
three generalised coupled XY models. We calculate the phase diagram and show
that, as the system is heated, the lightest strings first undergo the Hagedorn
transition despite the junctions. There is then a second, higher, critical
temperature above which infinite strings of all tensions, and junctions, exist.
Conversely, on cooling to low temperatures, only the lightest strings remain,
but they collapse into small loops.
