Spectropolarimetry of single and binary stars

dc.contributor.author	Harries, TJ
dc.date.accessioned	2018-01-12T09:30:28Z
dc.date.issued	2005-03
dc.description.abstract	Spectropolarimetry is a photon-hungry technique that will reach fruition in the 8-m telescope age. Here I summarize some of the stellar spectropolarimetric research that my collaborators and I have undertaken, with particular emphasis on the circumstellar environment of massive stars, symbiotic binaries, and star formation.	en_GB
dc.identifier.citation	Vol. 752, article 54	en_GB
dc.identifier.doi	10.1063/1.1893335
dc.identifier.uri	http://hdl.handle.net/10871/30920
dc.language.iso	en	en_GB
dc.publisher	AIP Publishing	en_GB
dc.rights	© 2005 American Institute of Physics	en_GB
dc.subject	Symbiotic binaries	en_GB
dc.subject	Binary stars	en_GB
dc.subject	Star formation	en_GB
dc.subject	Telescopes	en_GB
dc.title	Spectropolarimetry of single and binary stars	en_GB
dc.type	Article	en_GB
dc.date.available	2018-01-12T09:30:28Z
dc.description	This is the author accepted manuscript. The final version is available from AIP Publishing via the DOI in this record.	en_GB
dc.identifier.journal	AIP Conference Proceedings	en_GB