SIMBAD references

2018ApJ...859L..24H - Astrophys. J., 859, L24-L24 (2018/June-1)

The R-Process Alliance: 2MASS J09544277+5246414 the most actinide-enhanced R-II star known.

HOLMBECK E.M., BEERS T.C., ROEDERER I.U., PLACCO V.M., HANSEN T.T., SAKARI C.M., SNEDEN C., LIU C., LEE Y.S., COWAN J.J. and FREBEL A.

Abstract (from CDS):

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.

Abstract Copyright: © 2018. The American Astronomical Society. All rights reserved.

Journal keyword(s): Galaxy: halo - stars: abundances - stars: atmospheres - stars: individual: 2MASS J09544277+5246414 - stars: Population II

Simbad objects: 7

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