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20042009
most citedVariability of Disk Emission in Pre-Main Sequence and Related Stars. I. HD 31648 and HD 163296 - Isolated Herbig Ae Stars Driving Herbig-Haro Flows

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astro-ph200797 cited

Variability of Disk Emission in Pre-Main Sequence and Related Stars. I. HD 31648 and HD 163296 - Isolated Herbig Ae Stars Driving Herbig-Haro Flows

M. L. Sitko, W. J. Carpenter, R. L. Kimes +13

Infrared photometry and spectroscopy covering a time span of a quarter century are presented for HD 31648 (MWC 480) and HD 163296 (MWC 275). Both are isolated Herbig Ae stars that…

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-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-ph20067 cited

Visible and Near-Infrared Spectrophotometry of the Deep Impact Ejecta of Comet 9P/Tempel 1

Klaus W. Hodapp, Greg Aldering, Karen J. Meech +12

We have obtained optical spectrophotometry of the evolution of comet 9P/Tempel 1 after the impact of the Deep Impact probe, using the Supernova Integral Field Spectrograph (SNIFS)…

astro-ph200621 cited

Infrared observations of the 2006 outburst of the recurrent nova RS Ophiuchi: the early phase

A. Evans, T. Kerr, Bin Yang +20

We present infrared spectroscopy of the recurrent nova RS Ophiuchi, obtained 11.81, 20.75 and 55.71 days following its 2006 eruption. The spectra are dominated by hydrogen recombin…