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The spectrum of TMR-1C is consistant with a background star

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dc.contributor.author Terebey, S. en_US
dc.contributor.author Buren, D. Van en_US
dc.contributor.author Matthews, K. en_US
dc.contributor.author Padgett, D. en_US
dc.date.accessioned 2004-09-23T17:50:40Z
dc.date.available 2004-09-23T17:50:40Z
dc.date.issued 2000-05 en_US
dc.identifier.citation Astronomical journal, Vol. 119, No.5, 2000, pp. 2341- 2348 en_US
dc.identifier.citation Pasadena, CA, USA en_US
dc.identifier.clearanceno 00-0537 en_US
dc.identifier.uri http://hdl.handle.net/2014/14134
dc.description.abstract In a previous paper we proposed that there may be a population of runaway planets and brown dwarfs that formed via ejection from multiple-star systems. We further suggested TMR-1C as a candidate runaway protoplanet. en_US
dc.format.extent 189440 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other circumsteller matter planetsbrown drawf en_US
dc.title The spectrum of TMR-1C is consistant with a background star en_US


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