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epsilon Aurigae Campaign
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2010CHARAfig2.jpg
The bright star epsilon Aurigae eclipses every 27 years for nearly 2 years. The current 2009-2011 event was rich in research opportunities (see list of recent publications on main page). We made use of a wide array of ground based and space based telescopes to provide new insights into the nature of this enigmatic binary. Prior eclipses included 1983, 1956, 1929 and prior, where the nature of the eclipsing object was deduced, but firmly demonstrated by our interferometric imaging during 2009 and 2010.
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MidEclipseImages.png
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Breaking news on Twitterhttps://twitter.com/epsilon_Aurigae
Keep up with the eclipse campaign by monitoring real time updates on twitter.com/epsilon_Aurigae
See also papers on arXiv and May 2009 issue Sky & Telescope.
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Eclipse Monitoring Statushttp://mysite.du.edu/~rstencel/epsaur.htm
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SLIDESHOW
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Image Gallery for epsilon Aurigae
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Infrared Astronomy
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Projects in infrared observational astrophysics:
-- Spitzer photometry and spectra of epsilon Aur
-- Spitzer imaging of mass loss from highly evolved stars (MLHES)
-- AKARI studies of MLHES, joint with Dr. Ueta
-- IRTF MIRSI photometry of epsilon Aur
-- PTI evolved star data (van Belle)
-- J&H band photometry of evolved stars
-- VLTI MIDI data
-- additional new projects
If interested, contact Prof. Stencel, 409 P&A -
Adventures in Interferometry
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PTI pre-eclipse measurements of epsilon Aur (2008 ApJL)
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Interferometry tutorial paper, Monnier 2003 Rev. Prog. Phys.
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Telescopes and Instrumentation
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Mt. Evans observatory instrument upgrades
Student Astronomy Lab telescope control development
infrared instrumentation
interferometry
Contact Prof. Stencel, 409 P&A -
Other projects
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OUTREACH via DU's historic Chamberlin Observatory and Wings Museum/SpaceGrant:
see webpages www.du.edu/~rstencel/Chamberlin and www.du.edu/~rstencel/sps
LIGHT POLLUTION RESEARCH
ARCHAEOASTRONOMY
Contact Prof. Stencel, 409 P&A