A Study of the Planetary Nebula M57

Details A Study of the Planetary Nebula M57 A Study of the Planetary Nebula M57

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000spin.conf...37a&link_type=abstract

Materials Presented at the MU-SPIN Ninth Annual Users' Conference, p. 37

Computer Science

Planetary Nebulae, Ionization, A Stars, Imagery, Lower California (Mexico), Hubble Space Telescope

Scientific paper

We present an overview of the objects known as planetary nebulae. These emission nebulae are the end-product of the evolution of a dying star. our ground-based imagery is of the most famous of these objects, M57, also known as the Ring Nebula. Taken with the 2.12-meter telescope at San Pedro Matir in Baja, Mexico, these seeing-limited images show variations in ionization, density and temperature as a function of position in the nebula. Our ground-based imagery is compared to similar HST archival images.

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