Spectropolarimetry of single and binary stars
AIP Conference Proceedings
© 2005 American Institute of Physics
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.
This is the author accepted manuscript. The final version is available from AIP Publishing via the DOI in this record.
Vol. 752, article 54