CSM Epsilon Aurigae Project
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Transcript of CSM Epsilon Aurigae Project
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Sally SeebodeScience Educator SMUHSD
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Dean Drumheller, Steve Howell, Don Hoard, Sally Seebode, Darryl Stanford
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Take Data
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Hardware: Losmandy G11 Mount Meade 8” SCT @f/6.3 SBIG Self Guided Spectrograph (SGS) ST7XME cameraSoftware: TheSky 6- accurate mount control CCDSoft –image acquisition Maxim DL –image acquisition IRAF –spectra processing
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Raw Data Frame
Reduced Spectrum: standard methods using IRAF3800 – 4600A; 5800 – 6600A
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•EquivalentWidth
•Full Width Half
Max•Velocity
Minimum three students make measurements for each spectra, data averaged and plotted.
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Equivalent Widths (eqw): the width of a standardized rectangle representing the area of the absorption line. EQW relates to the flux.
Exaggerated for emphasis
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Full Width Half Max (FWHM): the width of the absorption line at half it’s maximum value. Changes in FWHM indicate velocity variations which relates to the temperature and composition of disk.
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Velocity: Measure the central wavelength to determine if object is moving toward or away from you and at what relative velocity.
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Small portion of data.
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“If I knew what I was looking for this would be much easier.”
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Student motivation more important than math/science literacy
IRAF hard to get on high school computers
Teacher collaboration helpful Lots of support for astronomy education: NITARP, AAVSO, Lift Off, Project Astro, etc.
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Variation in absorption of various elementsIndicative of varying density of the diskPossible Ring Structure
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Eqw minimumEqw maximumLeadbeater/Stencel plateaus
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Measure the days of a min or max
Find fraction of orbit this represents:width of ring = min or max days/(27.1 * 365)
Represent fraction angle (* 360)
Knowing the radius 18.1 AU, use small angle approximation (sin or tan) to find ring width
18.1 AU
Fraction of orbit= (20 days ) *360 (27.1*365)= 0.73
Ring Width = tan 0.73 * 18.1= 0.23 AU
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Ring mins and maxs are roughly 0.2 AU
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1990 – S. Ferluga: disk is actually a series of concentric rings with gaps between them (like rings of Saturn)
Ferluga (1990, A&A, 238, 270)
Our result predict an outer ring at a radius of 3.3AU, a wider ring with radius 2.8 AU, and two
small inner rings with a radius near 1.5 AU. These
two small rings may represent the one inner ring. Our results are similar to Ferluga’s
prediction.
Our result predict an outer ring at a radius of 3.3AU, a wider ring with radius 2.8 AU, and two
small inner rings with a radius near 1.5 AU. These
two small rings may represent the one inner ring. Our results are similar to Ferluga’s
prediction.
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Take data 2 or more times every week
Examine the spectra for more information: H alpha emission and absorption components
Changing molecular bands (CN, CH) FWHM interpretation