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dc.contributor.authorEasterla, Dylan
dc.contributor.authorMiller, Nathan A.
dc.date.accessioned2017-02-20T20:40:41Z
dc.date.available2017-02-20T20:40:41Z
dc.date.issued2017-02-20T20:40:41Z
dc.identifier.urihttp://digital.library.wisc.edu/1793/75845
dc.descriptionColor poster with text, diagrams, tables. images, and graphs.en
dc.description.abstractO and B-type stars are among the hottest, most luminous, and most massive stars in space, with O-stars comprising a mere 0.00003% of main sequence stars. Due to their extreme temperatures, appreciable amounts of ionizing radiation are emitted in the form of X-rays. O-stars generally follow the 10-7 Law, where one ten-millionth of the star’s luminosity comes out as X-rays. Using results from Berghofer et. al., our goal was to determine if the presence of exoplanets around O-stars could explain the scatter about the canonical 10-7 Law.en
dc.description.sponsorshipUniversity of Wisconsin--Eau Claire Office of Research and Sponsored Programsen
dc.language.isoen_USen
dc.relation.ispartofseriesUSGZE AS589;
dc.subjectO starsen
dc.subjectExtrasolar planetsen
dc.subjectPostersen
dc.titleHow Does the Presence of Extrasolar Planets Affect the X-ray Output of Hot Stars?en
dc.typePresentationen


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  • Student Research Day
    Posters of collaborative student/faculty research presented at Student Research Day

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