“…The Biella pluton, which is also known as the Valle del Cervo pluton, shows a concentric zoning in which the outer part consists of monzonite grading to syenite and the inner part consists of granite (Bigioggero et al, 1994 and references therein). The Biella and Traversella plutons are 30 Ma Bigioggero et al, 1994;Krummenacher & Evernden, 1960;Romer et al, 1996) and are emplaced in the internal Sesia-Lanzo Zone of the western Austroalpine domain (Figure 1(b)), which shows a pervasive structural imprint under eclogite facies conditions (Delleani, Spalla, Castelli, & Gosso, 2012, 2013Giorgetti, Tropper, Essene, & Peacor, 2000;Koons, 1986;Rubbo, Borghi, & Compagnoni, 1999;Tropper & Essene, 2002;Tropper, Essene, Sharp, & Hunziker, 1999;Zucali, 2002;Zucali & Spalla, 2011;Zucali, Spalla, & Gosso, 2002) dated 60 -80 Ma (Bussy, Venturini, Hunziker, & Martinotti, 1998;Cenki-Tok et al, 2011;Roda, Spalla, & Marotta, 2012;Rubatto, Gebauer, & Compagnoni, 1999;Rubatto et al, 2011) and related to the Alpine subduction. The Sesia-Lanzo Zone preserves scattered granulite to amphibolite facies relicts, which are related to Permian-Triassic lithospheric thinning that predates the Alpine convergence (Cenki-Tok et al, 2011;Lardeaux & Spalla, 1991;Rebay & Spalla, 2001;Spalla et al, 2014).…”