Abstract
There is increasing evidence that planets are ubiquitous, and may form around stars over a wide range of stellar masses. After a star dies, the planets may remain, and in some circumstances there may be a new epoch of planet formation after the main sequence. In this chapter, scenarios for the retention and formation of planets after star death, and the prospects for detection, including current known post-main sequence systems are discussed. Planets in the graveyard are, in many cases, easier observational targets than planets around main sequence stars. Different detection techniques may also be brought to bear, in some cases with much higher sensitivity, allowing the detection of low mass planets. Planets detected in the graveyard reflect the ‘live’ population of planets, and in some cases provide potentially strong constraints on planet formation processes, and the general planet population.
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Sigurdsson, S. (2008). Searching for Exoplanets in the Stellar Graveyard. In: Mason, J.W. (eds) Exoplanets. Springer Praxis Books. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-74008-7_8
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DOI: https://doi.org/10.1007/978-3-540-74008-7_8
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