Near-infrared H₂ emission as a probe of the global energetics and morphology of molecular clouds

dc.contributor.advisorNot available
dc.creatorLuhman, Michael L., 1964-
dc.date.accessioned2019-04-04T15:53:47Z
dc.date.available2019-04-04T15:53:47Z
dc.date.issued1995-08
dc.description.departmentAstronomyen_US
dc.format.mediumelectronicen_US
dc.identifier.urihttps://hdl.handle.net/2152/74156
dc.identifier.urihttp://dx.doi.org/10.26153/tsw/1287
dc.language.isoengen_US
dc.relation.ispartofUT Electronic Theses and Dissertationsen_US
dc.rightsCopyright © is held by the author. Presentation of this material on the Libraries' web site by University Libraries, The University of Texas at Austin was made possible under a limited license grant from the author who has retained all copyrights in the works.en_US
dc.rights.restrictionRestricteden_US
dc.subject.lcshMolecular clouds
dc.subject.lcshEmission spectroscopy
dc.subject.lcshH II regions (Astrophysics)
dc.subject.lcshInterstellar matter
dc.titleNear-infrared H₂ emission as a probe of the global energetics and morphology of molecular cloudsen_US
dc.typeThesisen_US
dc.type.genreThesisen_US
thesis.degree.departmentAstronomyen_US
thesis.degree.disciplineAstronomyen_US
thesis.degree.grantorUniversity of Texas at Austinen_US
thesis.degree.levelDoctoralen_US
thesis.degree.nameDoctor of Philosophyen_US
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