Difference between revisions of "IC 2118 Current Research Activities"
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==[[Chandra X-Ray Data]]== | ==[[Chandra X-Ray Data]]== | ||
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==[[Kitt Peak H-alpha Data]]== | ==[[Kitt Peak H-alpha Data]]== | ||
Revision as of 20:46, 12 December 2007
Contents
- 1 General Background on young stars
- 2 Color-Color Plots
- 3 Presentations, Posters, and Research Papers for IC2118
- 4 Information for Oil City High School meetings
- 5 Proposal for Radio Observations of T-Tauri Candidates in IC2118
- 6 Monitoring T-Tauri Stars using the Perth Obervatory Telescope
- 7 Chandra X-Ray Data
- 8 Kitt Peak H-alpha Data
- 9 USNO U, B, V, R, and I Data
- 10 Outflows or Jets
- 11 Multi Wavelength Composite Images
General Background on young stars
Color-Color Plots
Presentations, Posters, and Research Papers for IC2118
Information for Oil City High School meetings
Proposal for Radio Observations of T-Tauri Candidates in IC2118
Monitoring T-Tauri Stars using the Perth Obervatory Telescope
Chandra X-Ray Data
Kitt Peak H-alpha Data
In January of 2007 students from Oil City High School used the 0.9 Meter Telescope at Kitt peak to image regions of IC2118 in H-alpha.'
Matt Walentosky, Nick Kelley, Sandy Weiser were the students who went!!!!!!
USNO U, B, V, R, and I Data
U, B, V, R, and I data will be used to generate more accurate SEDs for the T-Tauri Candidates
Outflows or Jets
Visible outflows or jets are strong evidence that a candidate is indeed a T-Tauri Star
Multi Wavelength Composite Images
Images and Methods
FROM SPUCK 6/30/2007 See Image Below- IC 2118 3.6 µm (blue), 5.8 µm (green), 8.0 µm (red) tri-color composite generated using MaxIm DL. (By M. Heath, N. Kelley, P. Morton, M. Walentosky, S. Weiser – Oil City High School, Oil City, PA)
