dc.contributor.author | Frebel, Anna | |
dc.date.accessioned | 2020-04-17T19:15:58Z | |
dc.date.available | 2020-04-17T19:15:58Z | |
dc.date.issued | 2018-06 | |
dc.date.submitted | 2018-04 | |
dc.identifier.issn | 2041-8213 | |
dc.identifier.issn | 2041-8205 | |
dc.identifier.uri | https://hdl.handle.net/1721.1/124736 | |
dc.description.abstract | We report the discovery of a new actinide-boost star, 2MASS J09544277+5246414, originally identified as a very bright (V = 10.1), extremely metal-poor ([Fe/H] = -2.99) K giant in the LAMOST survey, and found to be highly r-process-enhanced (r-II; [Eu/Fe] = +1.28]), during the snapshot phase of the R-Process Alliance (RPA). Based on a high signal-to-noise ratio (S/N), high-resolution spectrum obtained with the Harlan J. Smith 2.7 m telescope, this star is the first confirmed actinide-boost star found by RPA efforts. With an enhancement of [Th/Eu] = +0.37, 2MASS J09544277+5246414 is also the most actinide-enhanced r-II star yet discovered, and only the sixth metal-poor star with a measured uranium abundance ([U/Fe] = +1.40). Using the Th/U chronometer, we estimate an age of 13.0 ± 4.7 Gyr for this star. The unambiguous actinide-boost signature of this extremely metal-poor star, combined with additional r-process-enhanced and actinide-boost stars identified by the RPA, will provide strong constraints on the nature and origin of the r-process at early times. ©2018 | en_US |
dc.publisher | American Astronomical Society | en_US |
dc.relation.isversionof | 10.3847/2041-8213/AAC722 | en_US |
dc.rights | Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. | en_US |
dc.source | The Astrophysical Journal Letters | en_US |
dc.title | The R-Process Alliance: 2MASS J09544277+5246414, the most actinide-enhanced R-II star known | en_US |
dc.type | Article | en_US |
dc.identifier.citation | Holmbeck, Erika M., et al., "The R-Process Alliance: 2MASS J09544277+5246414, the most actinide-enhanced R-II star known." Astrophysical journal. Letters 859, 2 (June 2018): letter 24 doi 10.3847/2041-8213/AAC722 ©2018 Author(s) | en_US |
dc.contributor.department | Massachusetts Institute of Technology. Department of Physics | en_US |
dc.contributor.department | MIT Kavli Institute for Astrophysics and Space Research | en_US |
dc.relation.journal | Astrophysical journal. Letters | en_US |
dc.eprint.version | Final published version | en_US |
dc.type.uri | http://purl.org/eprint/type/JournalArticle | en_US |
eprint.status | http://purl.org/eprint/status/PeerReviewed | en_US |
dc.date.updated | 2019-03-22T15:41:40Z | |
dspace.orderedauthors | Holmbeck, Erika M.; Beers, Timothy C.; Roederer, Ian U.; Placco, Vinicius M.; Hansen, Terese T.; Sakari, Charli M.; Sneden, Christopher; Liu, Chao; Lee, Young Sun; Cowan, John J.; Frebel, Anna | en_US |
dspace.embargo.terms | N | en_US |
dspace.date.submission | 2019-04-04T10:43:14Z | |
mit.journal.volume | 859 | en_US |
mit.journal.issue | 2 | en_US |
mit.license | PUBLISHER_POLICY | en_US |
mit.metadata.status | Complete | |