Determining 3-D Structure of Planetary Nebulae


Carthage College undergraduates will obtain deep images of several planetary nebulae, primarily in the OIII and V bands, to indentify structures both interior to the nebulae and in their extensive halos as part of an ongoing study of planetary nebula morphology. Following our successful study of NGC 2371/2, several addtional targets have been identified which present diverse structural characteristics, including NGC 7026, 2022 and 3242. The former is similar in structure to 2371/2; the latter two share common characteristics, with bipolar flow in a dual shell structure.

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Hillary Mathis, Site Manager
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950 N. Cherry Ave.
Tucson, AZ 85719
E-mail: hmathis@noao.edu
Telephone: (520) 318-8460
Fax: (520) 318-8417


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