activity
20052010
most citedThe Super-Soft X-ray Phase of Nova RS Ophiuchi 2006

126 citations · 454 across the 8 of their papers we have counts for

collaborators
Showing 2007Show all

6 papers · 1 filter

astro-ph200732 cited

Silicate dust in the environment of RS Ophiuchi following the 2006 eruption

A. Evans, C. E. Woodward, L. A. Helton +20

We present further Spitzer Space Telescope observations of the recurrent nova RS Ophiuchi, obtained over the period 208-430 days after the 2006 eruption. The later Spitzer IRS data…

astro-ph2007115 cited

The interaction of planetary nebulae and their AGB progenitors with the interstellar medium

C. J. Wareing, Albert A. Zijlstra, T. J. O'Brien

Interaction with the Interstellar Medium (ISM) cannot be ignored in understanding planetary nebula (PN) evolution and shaping. In an effort to understand the range of shapes observ…

astro-ph200775 cited

The SSS phase of RS Ophiuchi observed with Chandra and XMM-Newton I.: Data and preliminary Modeling

J. -U. Ness, S. Starrfield, A. P. Beardmore +13

The phase of Super-Soft-Source (SSS) emission of the sixth recorded outburst of the recurrent nova RS Oph was observed twice with Chandra and once with XMM-Newton. The observations…

astro-ph200723 cited

Spitzer and ground-based infrared observations of the 2006 eruption of RS Ophiuchi

A. Evans, C. E. Woodward, L. A. Helton +18

We present Spitzer Space Telescope and complementary ground-based infrared observations of the recurrent nova RS Ophiuchi, obtained over the period 64-111 days after the 2006 erupt…

astro-ph200723 cited

The Early Spectrophotometric Evolution of V1186 Scorpii (Nova Scorpii 2004 #1)

G. J. Schwarz, C. E. Woodward, M. F. Bode +19

We report optical photometry and optical through mid-infrared spectroscopy of the classical nova V1186 Sco. This slowly developing nova had an complex light curve with multiple sec…

astro-ph200730 cited

Swift observations of the 2006 outburst of the recurrent nova RS Ophiuchi: II. 1D hydrodynamical models of wind driven shocks

N. M. H. Vaytet, T. J. O'Brien, M. F. Bode

Following the early Swift X-ray observations of the latest outburst of the recurrent nova RS Ophiuchi in February 2006 (Paper I), we present new 1D hydrodynamical models of the sys…