activity
20012007
most citedInfrared spectroscopy of Nova Cassiopeiae 1993 (V705 Cas). IV. A closer look at the dust

67 citations · 193 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph2007★ 32 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-ph2006★ 35 cited

The Spitzer IRS view of V4334 Sgr (Sakurai's Object)

A. Evans, V. H. Tyne, J. Th. van Loon +11

We present an observation of the very late thermal pulse object V4334 Sgr (Sakurai's Object) with the Infrared Spectrometer (IRS) on the Spitzer Space Telescope. The emission from…

astro-ph2005★ 67 cited

Infrared spectroscopy of Nova Cassiopeiae 1993 (V705 Cas). IV. A closer look at the dust

A. Evans, V. H. Tyne, O. Smith +3

Nova Cassiopeiae 1993 (V705 Cas) was an archetypical dust-forming nova. It displayed a deep minimum in the visual light curve, and spectroscopic evidence for carbon, hydrocarbon an…

astro-ph2004★ 7 cited

The sub-millimetre evolution of V4334 Sgr (Sakurai's Object)

A. Evans, T. R. Geballe, V. H. Tyne +3

We report the results of monitoring of V4334 Sgr (Sakurai's Object) at 450 microns and 850 microns with SCUBA on the James Clerk Maxwell Telescope. The flux density at both wavelen…

astro-ph2004★ 16 cited

Warm high velocity CO in the wind of Sakurai's Object (= V4334 Sgr)

S. P. S. Eyres, T. R. Geballe, V. H. Tyne +3

We present UKIRT UIST spectra of Sakurai's Object (=V4334 Sgr) showing CO fundamental band absorption features around 4.7 microns. The line-centres are at heliocentric radial veloc…

astro-ph2004★ 36 cited

CO bands in V4334 Sgr (Sakurai's Object): the 12C/13C ratio

Ya. V. Pavlenko, T. R. Geballe, A. Evans +4

We present the results of our analysis of a high resolution (R ~ 30000) infrared spectrum of V4334 Sgr (Sakurai's Object) around the first overtone CO bands, obtained in 1998 July.…