W134: A New Pre-Main Sequence Double-Lined Spectroscopic Binary

dc.contributor.author	Padgett, Deborah L.	en_US
dc.contributor.author	Stapelfeldt, Karl R.	en_US
dc.date.accessioned	2004-10-06T15:38:50Z
dc.date.available	2004-10-06T15:38:50Z
dc.date.issued	1993	en_US
dc.identifier.clearanceno	93-1831	en_US
dc.identifier.uri	http://hdl.handle.net/2014/36296
dc.description.abstract	We report the discovery that the pre-main sequence star Walker 134 in the young cluster NGC 2264 is a double-lined spectroscopic binary.	en_US
dc.format.extent	2463904 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en_US
dc.subject.other	Walker 134 NGC 2264 spectroscopic binary G stars	en_US
dc.title	W134: A New Pre-Main Sequence Double-Lined Spectroscopic Binary	en_US