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

Terebey, S.; Buren,  D. Van; Matthews,  K.; Padgett,  D.

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