Structure of the Spiral Galaxy NGC 300
In 1963, Toomre built up classes of mass models for the highly flattened galaxies which have free parameters n, an and Cn. In order to keep the universal dimension, we adopt parameters bn(Cn2 = an2n+2*bn2/(n-1)!) instead of Cn. Series of the normalized Toomre's mass models (G = Vmax = Rmax = 1,...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
The Korean Space Science Society
1992-06-01
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| Series: | Journal of Astronomy and Space Sciences |
| Online Access: | http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1992/v9n1/OJOOBS_1992_v9n1_11.pdf |