X-ray Characteristics of the Hot Stars in Trumpler 14 and 16.

dc.contributor.advisorMiller, Nathan A.
dc.contributor.authorBilty, Kati
dc.date.accessioned2009-07-24T19:07:41Z
dc.date.available2009-07-24T19:07:41Z
dc.date.issued2009-07-24T19:07:41Z
dc.descriptionColor poster with text, images, and charts (Spring 2009)en
dc.description.abstractWe have obtained X-ray data from the orbiting Chandra X-ray observatory in order to investigate the hot stars in the star clusters Trumpler 14 and 16. Our data set contains a number of CCD images centered on two stars in the clusters (HD93250 and HD93129). After combining our images into a master image, a major initial task was determining which sources were detected and identifying them with previously cataloged optical sources. The dimmest sources have resulted in only a handful of photon counts and are therefore at the edge of detection for the instrument, making these detections difficult. The images of the brightest stars have resulted in thousands of photon counts.en
dc.description.sponsorshipUniversity of Wisconsin--Eau Claire Office of Research and Sponsored Programs.en
dc.identifier.urihttp://digital.library.wisc.edu/1793/35634
dc.language.isoen_USen
dc.relation.ispartofseriesUSGZE AS589en
dc.subjectEarly stars--Spectraen
dc.subjectSpectral irradiance--Measurementen
dc.subjectPhotons--Measurementen
dc.subjectPostersen
dc.titleX-ray Characteristics of the Hot Stars in Trumpler 14 and 16.en
dc.typePresentationen

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