| Goal |
|
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| Monitor
and correlate brightness variations with changes in spectra |
|
| of
astronomical objects. |
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| Projects |
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|
|
| 1.
Monitor BVRI and Wing band variability and spectra of stars using |
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| differential
single channel photometry and spectroscopy. |
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| 2.
Focus on RS CVn, late-type, irregular, and
g Cas (Be) variable stars. |
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| 3.
Develop baseline spectroscopic standards. |
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| 4.
Analyze spectral line profile shapes and shifts found in stellar,
extragalactic |
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| and solar
system objects. |
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