{"oa_version":"Published Version","_id":"15214","quality_controlled":"1","main_file_link":[{"open_access":"1","url":"https://doi.org/10.3847/1538-4357/ac45fc"}],"keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"publisher":"American Astronomical Society","issue":"2","article_processing_charge":"No","publication_identifier":{"eissn":["1538-4357"],"issn":["0004-637X"]},"intvolume":" 926","external_id":{"arxiv":["2110.03837"]},"tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"scopus_import":"1","month":"02","doi":"10.3847/1538-4357/ac45fc","publication_status":"published","year":"2022","title":"Reconstructing the Pleiades with Gaia EDR3","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","day":"18","citation":{"chicago":"Heyl, Jeremy, Ilaria Caiazzo, and Harvey B. Richer. “Reconstructing the Pleiades with Gaia EDR3.” The Astrophysical Journal. American Astronomical Society, 2022. https://doi.org/10.3847/1538-4357/ac45fc.","short":"J. Heyl, I. Caiazzo, H.B. Richer, The Astrophysical Journal 926 (2022).","mla":"Heyl, Jeremy, et al. “Reconstructing the Pleiades with Gaia EDR3.” The Astrophysical Journal, vol. 926, no. 2, 132, American Astronomical Society, 2022, doi:10.3847/1538-4357/ac45fc.","ama":"Heyl J, Caiazzo I, Richer HB. Reconstructing the Pleiades with Gaia EDR3. The Astrophysical Journal. 2022;926(2). doi:10.3847/1538-4357/ac45fc","apa":"Heyl, J., Caiazzo, I., & Richer, H. B. (2022). Reconstructing the Pleiades with Gaia EDR3. The Astrophysical Journal. American Astronomical Society. https://doi.org/10.3847/1538-4357/ac45fc","ieee":"J. Heyl, I. Caiazzo, and H. B. Richer, “Reconstructing the Pleiades with Gaia EDR3,” The Astrophysical Journal, vol. 926, no. 2. American Astronomical Society, 2022.","ista":"Heyl J, Caiazzo I, Richer HB. 2022. Reconstructing the Pleiades with Gaia EDR3. The Astrophysical Journal. 926(2), 132."},"language":[{"iso":"eng"}],"date_updated":"2024-04-02T07:27:52Z","status":"public","article_type":"original","publication":"The Astrophysical Journal","date_created":"2024-03-26T10:31:44Z","date_published":"2022-02-18T00:00:00Z","extern":"1","author":[{"full_name":"Heyl, Jeremy","first_name":"Jeremy","last_name":"Heyl"},{"id":"8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d","first_name":"Ilaria","full_name":"Caiazzo, Ilaria","last_name":"Caiazzo","orcid":"0000-0002-4770-5388"},{"last_name":"Richer","first_name":"Harvey B.","full_name":"Richer, Harvey B."}],"oa":1,"article_number":"132","volume":926,"abstract":[{"lang":"eng","text":"We search through an eight million cubic parsec volume surrounding the Pleiades star cluster and the Sun to identify both the current and past members of the Pleiades cluster within the Gaia EDR3 data set. We find nearly 1300 current cluster members and 289 former cluster candidates. Many of these candidates lie well in front of or behind the cluster from our point of view, so formerly they were considered cluster members, but their parallaxes put them more than 10 pc from the center of the cluster today. Over the past 100 Myr we estimate that the cluster has lost twenty percent of its mass including two massive white dwarf stars and the α2 Canum Venaticorum type variable star, 41 Tau. All three white dwarfs associated with the cluster are massive (1.01–1.06 M⊙) and have progenitors with main-sequence masses of about six solar masses. Although we did not associate any giant stars with the cluster, the cooling time of the oldest white dwarf of 60 Myr gives a firm lower limit on the age of the cluster."}],"type":"journal_article"}