Previous | Session 38 | Next
A. J. Weitenbeck, C.M. Anderson, A.D. Code, K.S. Bjorkman, M.R. Meade, B.L. Babler, J.J. Johnson, G.K. Fox, N.E.B. Zellner (U of Wisc Space Astronomy Lab)
Besides the stars with ISM polarization given in Anderson et al. (AJ 112, 2726) WUPPE obtained observations of several other stars which were targets of or were in the fields of targets of the other instruments on the ASTRO-2 Mission. For northern targets HD51285, HD31726, NGC2682 81 and BD+36 367 we will show observations made with WUPPE and HPOL (UW spectropolarimeter); for southern stars HD177999 and HD68049, we show only WUPPE data. These data are consistent with the general findings of Anderson et al. that the ISM polarization continues to decrease into the UV. WUPPE was supported by NASA contract 5-26777. www.sal.wisc.edu/~ajw/wupism2/postrMPL.txt.
If you would like more information about this abstract, please follow the link to www.sal.wisc.edu/~ajw/wupism2/postrMPL.tx. This link was provided by the author. When you follow it, you will leave the Web site for this meeting; to return, you should use the Back comand on your browser.
The author(s) of this abstract have provided an email address for comments about the abstract: ajw@sal.wisc.edu
Previous | Session 38 | Next
Bulletin of the American Astronomical Society, 37 #2
© 2005. The American Astronomical Soceity.