Scott Wolk
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Grant: Close
EPSILON AURIGAE IS A POSSIBLY UNSTABLE F SUPERGIANT STAR (OR POST-AGB STAR) WITH AN ENORMOUS DISK ORBITING ABOUT IT. THE DISK ECLIPSES THE STAR ONCE EVERY 27 YEARS PRODUCING A GRAY ECLIPSE LASTING NEARLY TWO YEARS. THIS GEOMETRY OFFERS A UNIQUE OPPORTUNIT
Open Date: 2010-01-14
Close Date: 2012-01-13
Grant: Close
SMITHSONIAN INSTITUTION - SMITHSONIAN ASTROPHYSICAL X-RAY OBSERVATIONS OF PLANETARY TRANSITS: SECONDARY ECLIPSE THE EFFECT OF STELLAR X-RAYS ON THEIR NEARBY GAS-GIANT PLANETS APPEAR TO BE SIGNIFICANT. THE X-RAYS HAVE BEEN CITED AT THE CAUSE OF EXCESS HEAT
Open Date: 2009-07-16
Close Date: 2011-12-31
Articles (12)
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2025
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2025
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2023
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2023
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2022
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2022
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2022
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2021
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2020
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2020
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2020
Collaborators (11)
Alan Jackson
Assistant Professor
Towson University
Edward Guinan
Professor
Villanova University
Sean Brittain
Professor
Clemson University
Jinyoung Serena Kim
Research Professor/Astronomer
University of Arizona
Joel Kastner
Professor
Rochester Institute of Technology
Scott Engle
Assistant Professor
Villanova University
Steven Silverberg
Smithsonian Astrophysical Observatory
Pragati Pradhan
Assistant Prof.
Embry-Riddle Aeronautical University
Nancy Remage Evans
Harvard-Smithsonian Center for Astrophysics
Massimo Marengo
Professor
Florida State University
Brandon C. Johnson
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