DYNAMICS OF NON-STEADY SPIRAL ARMS IN DISK GALAXIES

• Published in: The Astrophysical journal Vol. 763; no. 1; pp. 1 - 14
• Main Authors: Baba, Junichi, Saitoh, Takayuki R, Wada, Keiichi
• Format: Journal Article
• Language: English
• Published: United States 20-01-2013
• Subjects: ANGULAR MOMENTUM; ASTRONOMY; ASTROPHYSICS; ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; COMPUTERIZED SIMULATION; CORIOLIS FORCE; DAMPING; DENSITY; Disk galaxies; Dynamical systems; GALAXIES; KINETIC ENERGY; NONLINEAR PROBLEMS; Phases; RANDOMNESS; ROTATION; STARS; Three dimensional; THREE-DIMENSIONAL CALCULATIONS; TIME DEPENDENCE
• ISSN: 0004-637X; 1538-4357
• DOI: 10.1088/0004-637X/763/1/46

In order to understand the physical mechanisms underlying non-steady stellar spiral arms in disk galaxies, we analyzed the growing and damping phases of their spiral arms using three-dimensional N-body simulations. We confirmed that the spiral arms are formed due to a swing amplification mechanism that reinforces density enhancement as a seeded wake. In the damping phase, the Coriolis force exerted on a portion of the arm surpasses the gravitational force that acts to shrink the portion. Consequently, the stars in the portion escape from the arm, and subsequently they form a new arm at a different location. The resultant structure of the spiral arms in the N-body simulations is consistent with the observational nature of spiral galaxies. We conclude that the formation and structure of spiral arms in isolated disk galaxies can be reasonably understood by nonlinear interactions between a spiral arm and its constituent stars.