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...
Autore principale: | Magorrian, J |
---|---|
Natura: | Journal article |
Lingua: | English |
Pubblicazione: |
1999
|
Documenti analoghi
-
Stellar kinematical signatures of disc non-axisymmetries in the extended solar neighbourhood
di: Minchev I., et al.
Pubblicazione: (2012-02-01) -
Orbit-superposition models of discrete, incomplete stellar kinematics: application to the Galactic centre
di: Magorrian, J
Pubblicazione: (2019) -
Structure and dynamics of galaxies with a low surface-brightness disc - I. The stellar and ionized-gas kinematics
di: Pizzella, A, et al.
Pubblicazione: (2008) -
Constraining black hole masses from stellar kinematics by summing over all possible distribution functions
di: Magorrian, J
Pubblicazione: (2006) -
Central DM density cuspiness in LSB's: a stellar kinematics approach
di: Pizzella, A, et al.
Pubblicazione: (2004)