Scientific Drivers for SpectroPolarimetric INterferometry (SPIN)

Details Scientific Drivers for SpectroPolarimetric INterferometry (SPIN) Scientific Drivers for SpectroPolarimetric INterferometry (SPIN)

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001sf2a.conf..161c&link_type=abstract

Abstracts from SF2A-2001: Semaine de l'Astrophysique Francaise, meeting held in Lyon, France, May 28-June 1st, 2001, Eds.: F. Co

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I describe the prospective work undertaken on an interferometric technique using polarimetry called SPIN (Spectro-Polarimetric INterferometry). The use of SPIN can bring to interferometry an irreplaceable complement for locating and quantifying the mass loss closer to the star. I present first the applications for hot stars in linear polarization. In a second step, I stress particularly in the detection and the characterization of the magnetic fields by SPIN in circular polarization.

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