A large mass of H2 in the brightest cluster galaxy in Zwicky 3146

We present the Spitzer/IRS mid-infrared spectrum of the infrared-luminous (L(IR) = 4 x 10(11) L(circle dot)) brightest cluster galaxy (BCG) in the X-ray-luminous cluster Zwicky 3146 (Z3146; z = 0.29). The spectrum shows strong aromatic emission features, indicating that the dominant source of the infrared luminosity is star formation. The most striking feature of the spectrum, however, is the exceptionally strong molecular hydrogen (H(2)) emission lines, which seem to be shock-excited. The line luminosities and inferred warm H(2) gas mass (similar to 10(10) M(circle dot)) are 6 times larger than those of NGC 6240, the most H(2)-luminous galaxy at z <= 0.05. Together with the large amount of cold H(2) detected previously (similar to 10(11) M(circle dot)), this indicates that the Z3146 BCG contains disproportionately large amounts of both warm and cold H(2) gas for its infrared luminosity, which may be related to the intracluster gas cooling process in the cluster core.