Polarized Rings of Plantary Nebula NGC 6543 - The Cat's Eye

Claire Bendersky

Mount Holyoke College

CTIO REU/PIA 2005

Advisors: Hugo Schwarz and Romano Corradi





-What is a Planetary Nebula?

-What is Polarization?

-Data was gathered using ISIS

-Forbidden emission lines

-Personal

-Power Point





ABSTRACT:
Rings surrounding the core of planetary nebulae are a recent and unexpected discovery. Spectrapolarimetry was taken by ISIS, a double-armed, medium resolution spectrograph. The single to noise ratio was too low in all wavelengths, except in the [O III] (5007A) due to the nature of forbidden line emission. By plotting the angle and the degree of polarization vectors polarization from a central source becomes apparent, especially compared to the central source and halo which do not display polarization. Polarization in rings the imply they contain dust that scatters light from a central source. They are likely to be AGB remnants because their simple shape does not reflect the complex symmetry of the core.







Home ---Planetary Nebula ---Polarization ---ISIS ---Forbidden lines ---Personal



Questions? Comments? cnbender@mtholyoke.edu or cdersky@gmail.com