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20022009
most citedRadiation Pressure Dominate Regime of Relativistic Ion Acceleration

1k citations

Showing 2007Show all

24 papers · 1 filter

astro-ph2007131 cited

The carbon-rich type Ic SN 2007gr: the photospheric phase

S. Valenti, N. Elias-Rosa, S. Taubenberger +20

The first two months of spectroscopic and photometric monitoring of the nearby type Ic SN 2007gr are presented. The very early discovery (less than 5 days after the explosion) and…

astro-ph200714 cited

The 2003 Nov 14 occultation by Titan of TYC 1343-1865-1. II. Analysis of light curves

A. Zalucha, A. Fitzsimmons, J. L. Elliot +6

We observed a stellar occultation by Titan on 2003 November 14 from La Palma Observatory using ULTRACAM with three Sloan filters: u', g', and i' (358, 487, and 758 nm, respectively…

astro-ph2007

Mass loss and supernova progenitors

John Eldridge

We first discuss the mass range of type IIP SN progenitors and how the upper and lower limits impose interesting constraints on stellar evolution. Then we discuss the possible impl…

physics.chem-ph200719 cited

Isolated vibrational wavepackets in D2+: Defining superposition conditions and wavepacket distinguishability

W. A. Bryan, J. McKenna, E. M. L. English +9

Tunnel ionization of room-temperature D in an ultrashort (12 femtosecond) near infra-red (800 nm) pump laser pulse excites a vibrational wavepacket in the D2+ ions; a rotationa…

cond-mat.mtrl-sci200721 cited

Robust non-adiabatic molecular dynamics for metals and insulators

L. Stella, M. Meister, A. J. Fisher +1

We present a new formulation of the correlated electron-ion dynamics (CEID) scheme, which systematically improves Ehrenfest dynamics by including quantum fluctuations around the me…

astro-ph200722 cited

Radio Detection of Supernova 2004ip in the Circumnuclear Region of the Luminous Infrared Galaxy IRAS 18293-3413

M. A. Pérez-Torres, S. Mattila, A. Alberdi +6

We report a radio detection of supernova SN 2004ip in the circumnuclear region of the luminous infrared galaxy IRAS 18293-3413, using Very Large Array (VLA) observations at 8.4 GHz…