A new analysis of Spitzer observations of Comet 29P/Schwassmann–Wachmann 1

@article{Schambeau2015ANA,
  title={A new analysis of Spitzer observations of Comet 29P/Schwassmann–Wachmann 1},
  author={Charles A. Schambeau and Yanga R. Fern{\'a}ndez and Carey M. Lisse and Nalin H. Samarasinha and Laura M. Woodney},
  journal={Icarus},
  year={2015},
  volume={260},
  pages={60-72}
}
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References

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Spitzer Observations of the Dust Coma and Nucleus of 29P/Schwassmann-Wachmann 1
We obtained thermal images and spectra of comet and Centaur object 29P/Schwassmann-Wachmann 1 in late 2003 November. Images at 8, 24, and 70 μm reveal an extensive coma. At 24 μm the coma extends at
Spitzer Space Telescope Observations of the Nucleus of Comet 103P/Hartley 2
We have used the Spitzer Space Telescope InfraRed Spectrograph (IRS) 22-μm peakup array to observe thermal emission from the nucleus and trail of comet 103P/Hartley 2, the target of NASA’s Deep
INFRARED SPECTROSCOPY OF COMET 73P/SCHWASSMANN-WACHMANN 3 USING THE SPITZER SPACE TELESCOPE
We have used the Spitzer Space Telescope Infrared Spectrograph (IRS) to observe the 5–37 μm thermal emission of comet 73P/Schwassmann-Wachmann 3 (SW3), components B and C. We obtained low spectral
An Extended CO Source around Comet 29P/Schwassmann-Wachmann 1
Abstract Comet 29P/Schwassmann–Wachmann 1 has been studied during seven days in August 1998 with the SEST submillimeter telescope at ESO, La Silla, Chile. The CO ( J =2−1) emission at 230 GHz was
Nucleus properties of P/Schwassmann-Wachmann 1
Time series photometric measurements are presented of Comet P/Schwassmann-Wachmann 1 at a heliocentric distance of 5.886 AU when the comet possessed an extensive coma. The light curve shows a
The Activity of Comet 29P/Schwassmann–Wachmann 1 Monitored through Its CO J=2→1 Radio Line☆
Abstract The 230-GHz emission from CO was observed on 18 different days between 4 December 1996 and 1 January 1997 with the 15-m SEST antenna pointed toward Comet 29P/Schwassmann–Wachmann 1. The CO
Outburst activity in comets – II. A multiband photometric monitoring of comet 29P/Schwassmann–Wachmann 1
We have carried out a continuous multiband photometric monitoring of the nuclear activity of comet 29P/Schwassmann–Wachmann 1 from 2008 to 2010. Our main aim has been to study the outburst mechanism
Activity of Comet 29P/Schwassmann–Wachmann 1
The outbursts of the comet 29P/Schwassmann‐Wachmann 1: A new approach to the old problem
As far as outbursts activity is concerned, the 29P/Schwassmann-Wachmann 1 is the exceptional comet. This Centaur object shows quasi-regular flares with periodicities of 50 days (Trigo-Rodriguez et
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