tipa -- 10/7/2013

Collapse of a molecular cloud core to stellar densities: stellar core and outflow formation in radiation magnetohydrodynamics simulations

• Matthew R. Bate, Terrence S. Tricco, Daniel J. Price

Hot Galactic Winds Constrained by the X-Ray Luminosities of Galaxies

• Dong Zhang, Todd A. Thompson, Norman Murray, Eliot Quataert

The supernova CSS121015:004244+132827: a clue for understanding super-luminous supernovae

• S. Benetti, M. Nicholl, E. Cappellaro, A. Pastorello, S. J. Smartt, N. Elias-Rosa, A. J. Drake, L. Tomasella, M. Turatto, A. Harutyunyan, S. Taubenberger, S. Hachinger, A. Morales-Garoffolo, T.-W. Chen, M. Fraser, A. Gal-Yam, C. Inserra, P. Mazzali, M. L. Pumo, J. Sollermann, S. Valenti, D. R. Young

Discovering the Significance of 5 sigma

• Louis Lyons