Analysis of Co-spatial UV-optical HST/STIS Spectra of Planetary Nebula NGC 3242
This project sought to consider two important aspects of the planetary nebula NGC 3242 using new long-slit HST/STIS spectra. First, we investigated whether this object is chemically homogeneous by spatially dividing the slit into different regions and calculating the abundances of each region. The major result is that the elements of He, C, O, and
Miller, T. R. et al.
Fecha de publicación:
10
2016