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...
المؤلف الرئيسي: | Magorrian, J |
---|---|
التنسيق: | Journal article |
اللغة: | English |
منشور في: |
1999
|
مواد مشابهة
-
Stellar kinematical signatures of disc non-axisymmetries in the extended solar neighbourhood
حسب: Minchev I., وآخرون
منشور في: (2012-02-01) -
Orbit-superposition models of discrete, incomplete stellar kinematics: application to the Galactic centre
حسب: Magorrian, J
منشور في: (2019) -
Structure and dynamics of galaxies with a low surface-brightness disc - I. The stellar and ionized-gas kinematics
حسب: Pizzella, A, وآخرون
منشور في: (2008) -
Constraining black hole masses from stellar kinematics by summing over all possible distribution functions
حسب: Magorrian, J
منشور في: (2006) -
Central DM density cuspiness in LSB's: a stellar kinematics approach
حسب: Pizzella, A, وآخرون
منشور في: (2004)