The Daily Brew
Selected astro-ph abstracts for Friday 2014 August 8
- The Role of Turbulence in Neutrino-Driven Core-Collapse Supernova Explosions
Sean M. Couch, Christian D. Ott
[ arXiv:1408.1399v1 | PDF File ]
- The progenitors of calcium-rich transients are not formed in situ
Joe Lyman, Andrew Levan, Ross Church, Melvyn Davies, Nial Tanvir
[ arXiv:1408.1424v1 | PDF File ]
- DIRBE Comet Trails
Richard G. Arendt
[ arXiv:1408.1466v1 | PDF File ]
- The 0.1 < z < 1.65 evolution of the bright end of the [OII] luminosity function
Johan Comparat, Johan Richard, Jean-Paul Kneib, Olivier Ilbert, V. Gonzalez-Perez, Laurence Tresse, Julien Zoubian, Stephane Arnouts, Roland Bacon, Joel R. Brownstein, Carlton Baugh, Timothee Delubac, Anne Ealet, Stephanie Escoffier, Jian Ge, Eric Jullo, Cedric Lacey, Nicholas P. Ross, David Schlegel, Donald P. Schneider, Oliver Steele, Lidia Tasca, Christophe Yeche, Michael Lesser, Zhaoji Jiang, Yipeng Jing, Zhou Fan, Xiaohui Fan, Jun Ma, Jundan Nie, Jiali Wang, Zhenyu Wu, Tianmeng Zhang, Xu Zhou, Zhimin Zhou, Hu Zou
[ arXiv:1408.1523v1 | PDF File ]
- The Broad-Lined Type Ic SN 2012ap and the Nature of Relativistic Supernovae Lacking a Gamma-ray Burst Detection
D. Milisavljevic, R. Margutti, J. T. Parrent, A. M. Soderberg, R. A. Fesen, P. Mazzali, K. Maeda, N. E. Sanders, S. B. Cenko, J. M. Silverman, A. V. Filippenko, A. Kamble, S. Chakraborti, M. R. Drout, R. P. Kirshner, T. E. Pickering, K. Kawabata, T. Hattori, E. Y.Hsiao, M. D. Stritzinger, G. H. Marion, J. Vinko, J. C. Wheeler
[ arXiv:1408.1606v1 | PDF File ]
- There is a short gamma-ray burst prompt phase at the beginning of each long one
G. Calderone, G. Ghirlanda, G. Ghisellini, M.G. Bernardini, S. Campana, S. Covino, D'Avanzo, V. D'Elia, A. Melandri, R. Salvaterra, B. Sbarufatti, G. Tagliaferri
[ arXiv:1408.1608v1 | PDF File ]
- Search for bright nearby M dwarfs with Virtual Observatory tools
M. Aberasturi, J.A. Caballero, B. Montesinos, M.C. Gálvez-Ortiz, E. Solano, E.L. Martín
[ arXiv:1408.1611v1 | PDF File ]
- The Drop during Less than 300 days of a Dusty White Dwarf's Infrared Luminosity
S. Xu (1), M. Jura (1) ((1) UCLA)
[ arXiv:1408.1618v1 | PDF File ]
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