output
20022015
most citedRadiation Pressure Dominate Regime of Relativistic Ion Acceleration

1k citations

Showing 2007 · astro-phShow all

51 papers · 2 filters

astro-ph200751 cited

Optical observations of 23 distant Jupiter Family Comets, including 36P/Whipple at multiple phase angles

Colin Snodgrass, Stephen C. Lowry, Alan Fitzsimmons

We present photometry on 23 Jupiter Family Comets (JFCs) observed at large heliocentric distance, primarily using the 2.5m Isaac Newton Telescope (INT). Snap-shot images were taken…

astro-ph2007105 cited

The Outermost Ejecta of Type Ia Supernovae

Masaomi Tanaka, Paolo A. Mazzali, Stefano Benetti +6

The properties of the highest velocity ejecta of normal Type Ia supernovae (SNe Ia) are studied via models of very early optical spectra of 6 SNe. At epochs earlier than 1 week bef…

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-ph2007142 cited

The underluminous Type Ia Supernova 2005bl and the class of objects similar to SN 1991bg

S. Taubenberger, S. Hachinger, G. Pignata +24

Optical observations of the Type Ia supernova (SN Ia) 2005bl in NGC 4070, obtained from -6 to +66 d with respect to the B-band maximum, are presented. The photometric evolution is…

astro-ph2007500 cited

The effect of massive binaries on stellar populations and supernova progenitors

John J. Eldridge, Robert G. Izzard, Christopher A. Tout

We compare our latest single and binary stellar model results from the Cambridge STARS code to several sets of observations. We examine four stellar population ratios, the number o…