Abstract
The past decade brought direct evidence of the previously surmised exoplanetary systems. A variety of planetary system types exist: those around pulsars, around both young and old main-sequence stars (as evidenced by planetesimal disks of the Beta Pictoris-type), and the mature giant exoplanets found in radial velocity surveys. The surprising diversity of the exoplanetary systems is addressed by several theories of their origin.
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Artymowicz, P. (1999). Planetary Systems. In: Henrard, J., Ferraz-Mello, S. (eds) Impact of Modern Dynamics in Astronomy. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4527-5_31
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DOI: https://doi.org/10.1007/978-94-011-4527-5_31
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