Physical Parameters of Late Type Spiral Galaxies - III. Mass and Mass to Luminosity Ratio of NGC 7793
The mass distribution and other related quantities were calculated by fitting the observed rotation curve(Davoust and de Vaucouleur 1980) to Brandt and Belton's mass distribution model. One of n values for mass model is determined as 1.5(Vm = 95 km/s) and two pairs of them are determined as 0.8...
| Päätekijät: | , |
|---|---|
| Aineistotyyppi: | Artikkeli |
| Kieli: | English |
| Julkaistu: |
The Korean Space Science Society
1986-12-01
|
| Sarja: | Journal of Astronomy and Space Sciences |
| Linkit: | http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1986/v3n2/OJOOBS_1986_v3n2_103.pdf |