PAMELA results on the cosmic-ray antiproton flux from 60 MeV to 180 GeV in kinetic energy
- Authors: PAMELA Collaboration: O. Adriani, G. C. Barbarino, G. A. Bazilevskaya, R. Bellotti, M. Boezio, E. A. Bogomolov, L. Bonechi, M. Bongi, V. Bonvicini, S. Borisov, S. Bottai, A. Bruno, F. Cafagna, D. Campana, R. Carbone, P. Carlson, M. Casolino, G. Castellini, L. Consiglio, M. P. De Pascale, C. De Santis, N. De Simone, V. Di Felice, A. M. Galper, W. Gillard, L. Grishantseva, P. Hofverberg, G. Jerse, A. V. Karelin, S. V. Koldashov, S. Y. Krutkov, A. N. Kvashnin, A. Leonov, V. Malvezzi, L. Marcelli, A. G. Mayorov, W. Menn, V. V. Mikhailov, E. Mocchiutti, A. Monaco, N. Mori, N. Nikonov, G. Osteria, P. Papini, M. Pearce, P. Picozza, C. Pizzolotto, M. Ricci, S. B. Ricciarini, L. Rossetto, M. Simon, R. Sparvoli, P. Spillantini, Y. I. Stozhkov, A. Vacchi, E. Vannuccini, G. Vasilyev, S. A. Voronov, J. Wu, Y. T. Yurkin, G. Zampa, N. Zampa, V. G. Zverev
Supernovae Powered by Collapsar Accretion in Gamma-Ray Burst Sources
Direct Imaging of Bridged Twin Protoplanetary Disks in a Young Multiple Star
- Authors: Satoshi Mayama, Motohide Tamura, Tomoyuki Hanawa, Tomoaki Matsumoto, Miki Ishii, Tae-Soo Pyo, Hiroshi Suto, Takahiro Naoi, Tomoyuki Kudo, Jun Hashimoto, Shogo Nishiyama, Masayuki Kuzuhara, Masahiko Hayashi
On variations of the brightness of type Ia supernovae with the age of the host stellar population
- Authors: Brendan K. Krueger (1), Aaron P. Jackson (1), Dean M. Townsley (2), Alan C. Calder (1 and 3), Edward F. Brown (4), F. X. Timmes (5) ((1) The State University of New York - Stony Brook, (2) The University of Alabama, (3) New York Center for Computational Sciences, (4) Michigan State University, (5) Arizona State University)
No comments:
Post a Comment