next up previous
Next: Numerical Models of NGC4038/9 Up: A History of Mergers Previous: Vorontsov-Vel'yaminov (1959) and Arp

Toomre and Toomre (1972)

During the 1960's, Pfleiderer and Siedentopf investigated how spiral patterns in disk galaxies could be excited by gravitational interactions between disk galaxies and concluded that chance encounters between field galaxies are not sufficiently common enough to produce the observed population of spirals. However, they did produce, albeit in passing, the first plots of tail and bridge building.
This was followed in the early 1970's by a spate of papers, but one in particular stands out. Galactic Bridges and Tails by Toomre and Toomre (1972) is seen as many as the seminal paper in the field of galaxy interactions and mergers. Although it was not unusual at this time for a paper to be published that dealt with computer modeling of interacting galaxies, the publication of TT's paper was seen by many as a key turning point in the theory of interacting galaxies, triggering a true paradigm shift in the field. As will be highlighted in the next section, Galactic Bridges and Tails clearly established that bridges and tails - which for so long were the source of much heated debate and disagreement - were gravitational in nature. The paper comprehensively offered a very plausible and natural means to produce these characteristic features of interacting galaxies and indeed, through their discussion of related phenomena in the final section, the Toomres inspired a burst of new research. In particular, the discussion, Stoking the Furnace, preempted Larson&Tinsley's 1978 paper which showed the connection between starbursts and the merging of galaxies.


Chris Power
Thu Sep 16 20:11:54 BST 1999