Kinematical signatures of hidden stellar discs
The deprojection of the surface brightness distribution of an axisymmetric galaxy does not have a unique solution unless the galaxy is viewed precisely edge-on. I present an algorithm that finds the full range of smooth axisymmetric density distributions consistent with a given surface brightness di...
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| Materiálatiipa: | Journal article |
| Giella: | English |
| Almmustuhtton: |
1999
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