tipa -- 11/13/2015

Seeing double: the frequency and detectability of double-peaked superluminous supernova light curves

• M. Nicholl, S. J. Smartt

Are pulsars born with a hidden magnetic field?

• Alejandro Torres-Forné, Pablo Cerdá-Durán, José A. Pons, José A. Font

New reaction rates for improved primordial D/H calculation and the cosmic evolution of deuterium

• Alain Coc, Patrick Petitjean, Jean-Philippe Uzan, Elisabeth Vangioni, Pierre Descouvemont, Christian Illiadis, Richard Longland

Chandra observations of the elusive pulsar wind nebula around PSR B0656+14

• L. Bîrzan (Hamburger Sternwarte), G. G. Pavlov (PSU), O. Kargaltsev (George Washington University)

Extremely metal-poor stars from the cosmic dawn in the bulge of the Milky Way

• L. M. Howes, A. R. Casey, M. Asplund, S. C. Keller, D. Yong, D. M. Nataf, R. Poleski, K. Lind, C. Kobayashi, C. I. Owen, M. Ness, M. S. Bessell, G. S. Da Costa, B. P. Schmidt, P. Tisserand, A. Udalski, M. K. Szymański, I. Soszyński, G. Pietrzyński, K. Ulaczyk, Ł. Wyrzykowski, P. Pietrukowicz, J. Skowron, S. Kozłowski, P. Mróz