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dc.creatorJones, Michael R.
dc.date.accessioned 2007-05-09T17:58:35Z
dc.date.available 2007-05-09T17:58:35Z
dc.date.issued 1987
dc.identifier.citation Jones, Michael R.. "AN OPTICAL STUDY OF THE NUCLEI OF S0 STAR-BURST GALAXIES." (1987) Master’s Thesis, Rice University. http://hdl.handle.net/1911/13226.
dc.identifier.urihttp://hdl.handle.net/1911/13226
dc.description.abstract Optical observations of the nuclei of 10 S0 Markarian galaxies and two non-Markarian early type galaxies have been obtained with the McDonald Observatory 2.7m telescope. The spectra of 7 Markarian galaxies show deep Balmer absorption lines and stellar-like continua. The nuclear spectra of UGC 01157, 04902, 06570, and 12618 show strong (O II), (O III), and H$\beta$ emission lines analogous to normal H II regions. None of the galaxy continua show a featureless non-thermal component or (O I) $\lambda$ 6300 line emission typical of LINER activity. The continua of UGC 02093 and 07933 are similar to normal early type galaxies. Composite model spectra with decreasing birthrates, IMF exponents of $-1$, $-2.5$, and $-4$, and solar metallicity have been constructed from observed stellar spectra. Comparison of CaH + H$\varepsilon$ to CaK absorption line flux ratios measured in 5 star-burst galaxies to single star-bust episode models implies stellar population ages greater than 5 $\times$ 10$\sp9$ years.
dc.format.mimetype application/pdf
dc.language.iso eng
dc.subjectAstronomy
Astrophysics
dc.title AN OPTICAL STUDY OF THE NUCLEI OF S0 STAR-BURST GALAXIES
dc.type.genre Thesis
dc.type.material Text
thesis.degree.department Physics
thesis.degree.discipline Natural Sciences
thesis.degree.grantor Rice University
thesis.degree.level Masters
thesis.degree.name Master of Science


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