TOP Application for Coudé Feed telescope (spectroscopy), Fall 2007
There will be one observing run Nov 28-29. Applications are due Oct 24.
Background: Possible projects you may want to consider. You may also propose your own, but be sure to give sufficient detail about what you hope to study, and how you will carry out the project.
Spectroscopy of Variable Stars
Objective—correlate spectral changes in line strength, velocity, etc. with photometric variations to more fully understand the stars’ atmospheric structure. Examples: RV Tau stars,Mira variablesEclipsing Binaries
Objective—To measure the radial velocity changes in spectral lines in order to determine the orbital period, stellar masses, and other properties. Examples: Algol binaries, W UMa binariesPlanetary Nebula
Objective—To search for chemical differences in various PN and within the nebula itself to aid in studies of PN formation Examples: NGC6543, Ring Nebula
Other examples (previous years’ successful projects):
- Spectroscopy of the Planet Mars;
- Spectroscopy of suspected Metal Poor Stars;
- Spectral analysis of Planetary Nebulae
- Spectroscopy of the planets Jupiter, Saturn, Uranus and Neptune
- Analyzing Spectra of Stars on the Hertzsprung—Russell diagram
- Spectroscopy of Comets
: : : : : :
The Astronomy RBSE program is administered by the National Optical Astronomy Observatory with funds from the National Science Foundation.