How does it happen that billions of stars can cooperate to produce the beautiful spirals that characterize so many galaxies, including ours? This book presents a theory of spiral structure that has been developed over the past three decades under the continuous stimulus of new observational studies. The theory unfolds in a way that can be grasped by any reader with an undergraduate science background who is interested in astronomy, as well as by graduate students and scientists actively involved in astronomy or related subjects who want to see the "backbone" and the physical content of the theory. The foundations of this theoretical framework were laid in the early 1960s, following the pioneering work of B. Lindblad. C. C. Lin had already c...
The dynamics of stars and gas appear markedly different in flocculent, tidally induced and quasi-sta...
Context. Several spiral galaxies, as beautifully exhibited by the case of NGC 6946, display a promin...
[[abstract]]We undertake a semiempirical study of the spiral patterns of three model galaxies constr...
The dynamics of spiral galaxies is a gold-mine of challenging problems for the astrophysicist and th...
With the arrival of computers, plasma physics and several fresh investigators by the early 1960s, un...
[[abstract]]The density-wave theory of galactic spirals is developed in a form slightly more general...
[[abstract]]Axisymmetric models of disk galaxies taken together with the density wave theory allow o...
In this thesis, we try to prove the stability of spiral arms using the density wave theory. This the...
[[abstract]]It is pointed out that the theory of spiral density waves, invented to explain the spira...
Three theoretical problems concerning the large scale structure of disk galaxies in general, and the...
International audienceThis paper is the third in a series of articles devoted to the determination o...
The generation of transient spiral waves by swing-amplification in self-gravitating disks is now reg...
Spiral structure is the most distinctive feature of disk galaxies and yet debate persists about whic...
Studying galaxy structures using different wavebands enables us to observe a varietyof intrinsic gal...
Spiral structure is the most distinctive feature of disk galaxies and yet debate persists about whic...
The dynamics of stars and gas appear markedly different in flocculent, tidally induced and quasi-sta...
Context. Several spiral galaxies, as beautifully exhibited by the case of NGC 6946, display a promin...
[[abstract]]We undertake a semiempirical study of the spiral patterns of three model galaxies constr...
The dynamics of spiral galaxies is a gold-mine of challenging problems for the astrophysicist and th...
With the arrival of computers, plasma physics and several fresh investigators by the early 1960s, un...
[[abstract]]The density-wave theory of galactic spirals is developed in a form slightly more general...
[[abstract]]Axisymmetric models of disk galaxies taken together with the density wave theory allow o...
In this thesis, we try to prove the stability of spiral arms using the density wave theory. This the...
[[abstract]]It is pointed out that the theory of spiral density waves, invented to explain the spira...
Three theoretical problems concerning the large scale structure of disk galaxies in general, and the...
International audienceThis paper is the third in a series of articles devoted to the determination o...
The generation of transient spiral waves by swing-amplification in self-gravitating disks is now reg...
Spiral structure is the most distinctive feature of disk galaxies and yet debate persists about whic...
Studying galaxy structures using different wavebands enables us to observe a varietyof intrinsic gal...
Spiral structure is the most distinctive feature of disk galaxies and yet debate persists about whic...
The dynamics of stars and gas appear markedly different in flocculent, tidally induced and quasi-sta...
Context. Several spiral galaxies, as beautifully exhibited by the case of NGC 6946, display a promin...
[[abstract]]We undertake a semiempirical study of the spiral patterns of three model galaxies constr...