| dc.contributor.advisor | Paul C. Joss. | en_US |
| dc.contributor.author | Collins, Charles Aloysius | en_US |
| dc.date.accessioned | 2007-11-16T14:32:32Z | |
| dc.date.available | 2007-11-16T14:32:32Z | |
| dc.date.copyright | 1995 | en_US |
| dc.date.issued | 1996 | en_US |
| dc.identifier.uri | http://hdl.handle.net/1721.1/39608 | |
| dc.description | Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 1996. | en_US |
| dc.description | Includes bibliographical references (p. 117-118). | en_US |
| dc.description.statementofresponsibility | by Charles Aloysius Collins. | en_US |
| dc.format.extent | 118 p. | en_US |
| dc.language.iso | eng | en_US |
| dc.publisher | Massachusetts Institute of Technology | en_US |
| dc.rights | M.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.uri | http://dspace.mit.edu/handle/1721.1/7582 | |
| dc.subject | Physics | en_US |
| dc.title | The effects of non-vanishing stellar size in binary-single star scattering | en_US |
| dc.type | Thesis | en_US |
| dc.description.degree | Ph.D. | en_US |
| dc.contributor.department | Massachusetts Institute of Technology. Department of Physics | |
| dc.identifier.oclc | 34592590 | en_US |