Add to ORKGAbstract: The disks of galaxies are primarily stellar systems, and fundamentally dynamical entities. Thus, to fully understand galactic disks, we must study their stellar kinematics as well as their morphologies. Observational techniques have now advanced to a point where quite detailed stellar-kinematic information can be extracted from spectral observations. This review presents three illustrative examples of analyses that make use of such information to study the formation and evolution of these systems: the derivation of the pattern speed of the bar in NGC 936; the calculation of the complete velocity ellipsoid of random motions in NGC 488; and the strange phenomenon of counter-rotation seen in NGC 3593
n this thesis several aspects of the stellar kinematics in disk galaxies have been addressed. Due to...
n this thesis several aspects of the stellar kinematics in disk galaxies have been addressed. Due to...
n this thesis several aspects of the stellar kinematics in disk galaxies have been addressed. Due to...
Abstract: The disks of galaxies are primarily stellar systems, and fundamentally dynamical entities....
Abstract: The disks of galaxies are primarily stellar systems, and fundamentally dynamical entities....
Abstract: The disks of galaxies are primarily stellar systems, and fundamentally dynamical entities....
Abstract: The disks of galaxies are primarily stellar systems, and fundamentally dynamical entities....
Abstract. The disks of galaxies are primarily stellar systems, and fun-damentally dynamical entities...
Looking up, at night, one can immediately notice that the universe is almost empty. On a bright nigh...
Looking up, at night, one can immediately notice that the universe is almost empty. On a bright nigh...
Looking up, at night, one can immediately notice that the universe is almost empty. On a bright nigh...
Looking up, at night, one can immediately notice that the universe is almost empty. On a bright nigh...
We present deep optical long-slit spectra of 17 edge-on spiral galaxies of intermediate to late morp...
We present deep optical long-slit spectra of 17 edge-on spiral galaxies of intermediate to late morp...
We present deep optical long-slit spectra of 17 edge-on spiral galaxies of intermediate to late morp...
n this thesis several aspects of the stellar kinematics in disk galaxies have been addressed. Due to...
n this thesis several aspects of the stellar kinematics in disk galaxies have been addressed. Due to...
n this thesis several aspects of the stellar kinematics in disk galaxies have been addressed. Due to...
Abstract: The disks of galaxies are primarily stellar systems, and fundamentally dynamical entities....
Abstract: The disks of galaxies are primarily stellar systems, and fundamentally dynamical entities....
Abstract: The disks of galaxies are primarily stellar systems, and fundamentally dynamical entities....
Abstract: The disks of galaxies are primarily stellar systems, and fundamentally dynamical entities....
Abstract. The disks of galaxies are primarily stellar systems, and fun-damentally dynamical entities...
Looking up, at night, one can immediately notice that the universe is almost empty. On a bright nigh...
Looking up, at night, one can immediately notice that the universe is almost empty. On a bright nigh...
Looking up, at night, one can immediately notice that the universe is almost empty. On a bright nigh...
Looking up, at night, one can immediately notice that the universe is almost empty. On a bright nigh...
We present deep optical long-slit spectra of 17 edge-on spiral galaxies of intermediate to late morp...
We present deep optical long-slit spectra of 17 edge-on spiral galaxies of intermediate to late morp...
We present deep optical long-slit spectra of 17 edge-on spiral galaxies of intermediate to late morp...
n this thesis several aspects of the stellar kinematics in disk galaxies have been addressed. Due to...
n this thesis several aspects of the stellar kinematics in disk galaxies have been addressed. Due to...
n this thesis several aspects of the stellar kinematics in disk galaxies have been addressed. Due to...