Show simple item record

dc.contributor.advisorMushotzky, Richard Fen_US
dc.contributor.advisorLeventhal, Marvinen_US
dc.contributor.authorBaumgartner, Wayneen_US
dc.date.accessioned2004-06-04T05:29:04Z
dc.date.available2004-06-04T05:29:04Z
dc.date.issued2004-04-30en_US
dc.identifier.urihttp://hdl.handle.net/1903/1387
dc.description.abstractThe first part of this dissertation deals with the oxygen abundance of the Milky Way interstellar medium. Previous measurements had shown that oxygen in the ISM was depleted compared to its abundance in the sun. This dissertation presents new measurements of the ISM oxygen abundance taken in the X-ray band by observing the oxygen 0.6 keV photoionization K-edge in absorption towards 10 galaxy clusters. These measurements show that the ISM oxygen abundance is 0.9 solar, much greater than earlier depleted values. The oxygen abundance is found to be uniform across our 10 lines of sight, showing that it is not dependent on the depth of the hydrogen column. This implies that the galactic oxygen abundance does not depend on density, and that it is the same in dense clouds and in the more diffuse ISM. The next part of the dissertation measures elemental abundances in the galaxy clusters themselves. The abundances of the elements iron, silicon, sulfur, calcium, argon, and nickel are measured using the strong resonance K-shell emission lines in the X-ray band. Over 300 clusters from the ASCA archives are analyzed with a joint fitting procedure to improve the S/N ratio and provide the first average abundance results for clusters as a function of mass. The alpha elements silicon, sulfur, argon and calcium are not found to have similar abundances as expected from their supposed common origin. Also, no combination of SN Ia and SN II yields can account for the cluster abundance ratios, perhaps necessitating a contribution from a cosmologically early generation of massive population III stars. The last part of this dissertation details the development of the Cadmium Zinc Telluride (CZT) detectors on the InFOCuS hard X-ray telescope. InFOCuS is a balloon-borne imaging spectrometer that incorporates multi-layer coated grazing-incidence optics and CZT detectors. These detectors are well suited for hard X-ray astronomy because their large bandgap and high atomic number allow for efficient room temperature detection of photons in the 20-150 keV band. The InFOCuS CZT detectors achieve an energy resolution of 4.0 keV. A 2000 flight to measure the inflight background is discussed, as well as the results of a 2001 flight to observe Cyg X-1.en_US
dc.format.extent4165666 bytes
dc.format.extent4165666 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypeapplication/pdf
dc.language.isoen_US
dc.titleElemental Abundances via X-ray Observations of Galaxy Clusters and the InFOCuS Hard X-ray Telescopeen_US
dc.typeDissertationen_US
dc.relation.isAvailableAtDigital Repository at the University of Marylanden_US
dc.relation.isAvailableAtUniversity of Maryland (College Park, Md.)en_US
dc.contributor.departmentAstronomyen_US
dc.subject.pqcontrolledPhysics, Astronomy and Astrophysicsen_US
dc.subject.pquncontrolledGalaxy Clustersen_US
dc.subject.pquncontrolledElemental Abundancesen_US
dc.subject.pquncontrolledX-ray Astronomyen_US
dc.subject.pquncontrolledX-ray Telescopeen_US
dc.subject.pquncontrolledCZTen_US


Files in this item

Thumbnail
Thumbnail

This item appears in the following Collection(s)

Show simple item record