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 |