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dc.contributor.authorPaley, Elizabeth Sara, 1967-
dc.creatorPaley, Elizabeth Sara, 1967-en_US
dc.date.accessioned2013-03-28T10:29:27Z
dc.date.available2013-03-28T10:29:27Z
dc.date.issued1989en_US
dc.identifier.urihttp://hdl.handle.net/10150/277118
dc.description.abstractA sample of 170 sources from the IRAS Point Source Catalog (PSC) having
dc.description.abstractb
dc.description.abstract≥ 40°, 100μm flux F₄ ≥ 2.5 Jy, and upper limit fluxes at 12, 25 and 60μm was studied on POSS and ESO photographic plates. 151 of these sources are identified as 'infrared cirrus,' thirteen as galaxies, and one as a planetary nebula; four sources lie in the Small Magellanic Cloud (SMC), and the remaining source is Saturn. Accurate infrared fluxes were obtained for 29 cirrus sources, the galaxies, and the planetary nebula. The colors of the cirrus sources support the hypothesis that the radiation is coming from a mixture of large, cool grains and Polycyclic Aromatic Hydrocarbons (PAHs), with large variation in relative abundances. Optical colors and surface brightness were obtained for one cirrus cloud using data from the CCD Transit Instrument on Kitt Peak.
dc.language.isoen_USen_US
dc.publisherThe University of Arizona.en_US
dc.rightsCopyright © is held by the author. Digital access to this material is made possible by the University Libraries, University of Arizona. Further transmission, reproduction or presentation (such as public display or performance) of protected items is prohibited except with permission of the author.en_US
dc.subjectInfrared astronomy -- Observations.en_US
dc.subjectInfrared sources -- Observations.en_US
dc.subjectAstronomy -- Remote sensing.en_US
dc.titleAn infrared and optical study of bright IRAS point sources of minimum apparent temperatureen_US
dc.typetexten_US
dc.typeThesis-Reproduction (electronic)en_US
dc.identifier.oclc23296371en_US
thesis.degree.grantorUniversity of Arizonaen_US
thesis.degree.levelmastersen_US
dc.identifier.proquest1338081en_US
thesis.degree.disciplineGraduate Collegeen_US
thesis.degree.disciplineAstronomyen_US
thesis.degree.nameM.S.en_US
dc.identifier.bibrecord.b17614831en_US
refterms.dateFOA2018-06-16T10:15:55Z
html.description.abstractA sample of 170 sources from the IRAS Point Source Catalog (PSC) having
html.description.abstractb
html.description.abstract≥ 40°, 100μm flux F₄ ≥ 2.5 Jy, and upper limit fluxes at 12, 25 and 60μm was studied on POSS and ESO photographic plates. 151 of these sources are identified as 'infrared cirrus,' thirteen as galaxies, and one as a planetary nebula; four sources lie in the Small Magellanic Cloud (SMC), and the remaining source is Saturn. Accurate infrared fluxes were obtained for 29 cirrus sources, the galaxies, and the planetary nebula. The colors of the cirrus sources support the hypothesis that the radiation is coming from a mixture of large, cool grains and Polycyclic Aromatic Hydrocarbons (PAHs), with large variation in relative abundances. Optical colors and surface brightness were obtained for one cirrus cloud using data from the CCD Transit Instrument on Kitt Peak.


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