A steady-state calculation of column densities of interstellar species toward [Zeta] Ophiuchi, [Omicron] Persei and Lynds 134

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dc.contributor.advisor Mitchell, George Ferguson, 1941-
dc.creator Funakawa, Hironobu
dc.date.accessioned 2011-05-09T12:31:21Z
dc.date.available 2011-05-09T12:31:21Z
dc.date.issued 1978
dc.identifier.other QB790 F86
dc.identifier.uri http://library2.smu.ca/xmlui/handle/01/22057
dc.description ii, 107 leaves : charts ; 28 cm.
dc.description Bibliography: leaves 59-60.
dc.description Online version unavailable; print version available from Patrick Power Library.
dc.description.abstract Calculations of column densities of some 100 interstellar species based on a steady-state analysis are carried out for interstellar clouds towards [zeta] Oph, [omicron] Per, and Lynds 134, using appropriate cloud models and physical conditions. The observed column densities of CH, OH, and CO are well reproduced by calculations. However, the calculated column densities of CH[superscript +] and C[subscript 2] show somewhat large discrepancies from the observed values. No explanation was found for these discrepancies. Column densities of species including [superscript 13]C are also calculated for L134.
dc.language.iso en
dc.publisher Halifax, N.S. : Saint Mary's University
dc.subject.lcc QB790
dc.subject.lcsh Interstellar matter
dc.title A steady-state calculation of column densities of interstellar species toward [Zeta] Ophiuchi, [Omicron] Persei and Lynds 134
dc.type Text
thesis.degree.name Master of Science in Astronomy
thesis.degree.level Masters
thesis.degree.discipline Astronomy
thesis.degree.grantor Saint Mary's University (Halifax, N.S.)


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