Second generation planet

A second generation planet is a type of exoplanet that forms in a binary star system when one of the stars becomes a red giant and mass transfers from it to an accretion disk around the other star where the planet can form.^[1]^[2]

References

^ Perets, Hagai P. (27 January 2010). "Second generation planets". arXiv:1001.0581 [astro-ph.EP].
^ Kluska, J.; Van Winckel, H.; Coppée, Q.; Oomen, G.-M.; Dsilva, K.; Kamath, D.; Bujarrabal, V.; Min, M. (February 2022). "A population of transition disks around evolved stars: Fingerprints of planets: Catalog of disks surrounding Galactic post-AGB binaries". Astronomy & Astrophysics. 658: A36. arXiv:2201.13155. Bibcode:2022A&A...658A..36K. doi:10.1051/0004-6361/202141690.

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[Perets_2010-1] Perets, Hagai P. (27 January 2010). "Second generation planets". arXiv:1001.0581 [astro-ph.EP].

[Kluska_et_al._2022-2] Kluska, J.; Van Winckel, H.; Coppée, Q.; Oomen, G.-M.; Dsilva, K.; Kamath, D.; Bujarrabal, V.; Min, M. (February 2022). "A population of transition disks around evolved stars: Fingerprints of planets: Catalog of disks surrounding Galactic post-AGB binaries". Astronomy & Astrophysics. 658: A36. arXiv:2201.13155. Bibcode:2022A&A...658A..36K. doi:10.1051/0004-6361/202141690.

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