UV Spectropolarimetry of the Eclipsing Binary V356 SGR

Details UV Spectropolarimetry of the Eclipsing Binary V356 SGR UV Spectropolarimetry of the Eclipsing Binary V356 SGR

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aas...191.4511l&link_type=abstract

American Astronomical Society, 191st AAS Meeting, #45.11; Bulletin of the American Astronomical Society, Vol. 29, p.1282

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The massive binary system V356 Sgr has been observed spectropolarimetrically in the UV with the Hubble Space Telescope Faint Object Spectrometer at two epochs. In a previous poster we have presented the results from 1300-1600 AA which showed evidence of polarization from Rayleigh Scattering as well as asymmetric electron scattering. Previous data suffered from poor phase coverage, and only outside of eclipse UV spectropolarimetry was available. New polarimetric observations both inside and outside of eclipse have been obtained for the 1600-2300 AA region. These data show clear evidence of intrinsic polarization associated with the primary or mass gaining star. We report on the results obtained from an analysis of these FOS data and comment on implications for current models of this system.

Affiliated with

Also associated with

No associations

Rating

UV Spectropolarimetry of the Eclipsing Binary V356 SGR does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with UV Spectropolarimetry of the Eclipsing Binary V356 SGR, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and UV Spectropolarimetry of the Eclipsing Binary V356 SGR will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1174052