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dc.contributor.advisorScott Wolk and Tyler Bourke.en_US
dc.contributor.authorVigil, Miquela, 1981-en_US
dc.contributor.otherMassachusetts Institute of Technology. Dept. of Earth, Atmospheric, and Planetary Sciences.en_US
dc.date.accessioned2005-09-27T17:19:52Z
dc.date.available2005-09-27T17:19:52Z
dc.date.issued2004en_US
dc.identifier.urihttp://hdl.handle.net/1721.1/28615
dc.descriptionThesis (S.M.)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric, and Planetary Sciences, 2004.en_US
dc.description"June 2004."en_US
dc.descriptionIncludes bibliographical references (leaves 41-42).en_US
dc.description.abstractI present 1.2 mm observations of the HII regions RCW 38, RCW 36, and RCW 108 which reveal the distributions of dust associated with the three regions. The dust emission in RCW 38 exhibits a ring like structure centered around an O-star. A bright knot in the ring was determined to contain 15% of the total dust by mass in the region and roughly coincided with regions of high emission at various infrared wavelengths as well as 6 cm continuum emission. The dust emission in RCW 36 extended along a ridge with a bright clump in the north of the ridge containing 70% of the mass of the entire cluster. The dust emission in RCW 108 is concentrated in a single tight knot with a faint extension to the south. The dust emission is compared to the infrared and radio emissions to attempt to describe the characteristics of possible areas of active star formation.en_US
dc.description.statementofresponsibilityMiquela Vigil.en_US
dc.format.extent42 leavesen_US
dc.format.extent2137660 bytes
dc.format.extent2140295 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypeapplication/pdf
dc.language.isoen_US
dc.publisherMassachusetts Institute of Technologyen_US
dc.rightsM.I.T. theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission. See provided URL for inquiries about permission.en_US
dc.rights.urihttp://dspace.mit.edu/handle/1721.1/7582
dc.subjectEarth, Atmospheric, and Planetary Sciences.en_US
dc.titleStar formation in the HII regions RCW 38, RCW 36, and RCW 108en_US
dc.typeThesisen_US
dc.description.degreeS.M.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
dc.identifier.oclc57560440en_US


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