Comet Hale-Bopp
For my first postdoc at Wisconsin, I analyzed Fabry-Pérot imaging
and spectroscopic data of comet Hale-Bopp. The project was part of a
large observing campaign led by Frank
Scherb involving several instruments and telescopes. The data analysis
effort was led by Walt
Harris.
We wrote a description of the Wisconsin
observations for the proceedings of IAU colloquium No. 186. Also
in the proceedings is a preliminary look at
high resolution spectra of H-alpha data and a look at collisional effects
in the OH distribution of the coma. With some modeling work, the H-alpha
observations may be able to shed some light on why comet Hale-Bopp had so
much [OI] emission. A paper describing that problem and some potential
solutions to was published in the Astrophysical Journal and
can be downloaded here. Several
other papers have come out of the Hale-Bopp which are listed in my CV. Although a little
out of date, part
of my homepage back in Wisconsin has more information on the project,
including a link to Chris Anderson's
Hale-Bopp page.
- Calculation of Wisconsin
H-alpha Mapper (WHAM) field rotation
- Modeling of spectroscopic and imaging modes of dual-etalon Fabry-Pérot
spectrometers
- Solar spectrum modeling
- Successful empirical coma gas distribution modeling, including quenching
- Publication of 3 first-author papers
- Editing of several other papers
Jeffrey P. Morgenthaler
2008-12-17