2021ApJ...908..247W


Query : 2021ApJ...908..247W

2021ApJ...908..247W - Astrophys. J., 908, 247-247 (2021/February-3)

An unsupervised method for identifying X-enriched stars directly from spectra: Li in LAMOST.

WHEELER A.J., HOGG D.W. and NESS M.

Abstract (from CDS):

Stars with peculiar element abundances are important markers of chemical enrichment mechanisms. We present a simple method, tangent space projection (TSP), for the detection of X-enriched stars, for arbitrary elements X, even from blended lines. Our method does not require stellar labels, but instead directly estimates the counterfactual unenriched spectrum from other unlabeled spectra. As a case study, we apply this method to the 6708 Å Li doublet in LAMOST DR5, identifying 8428 Li-enriched stars seamlessly across evolutionary state. We comment on the explanation for Li-enrichment for different subpopulations, including planet accretion, nonstandard mixing, and youth.

Abstract Copyright: © 2021. The American Astronomical Society. All rights reserved.

Journal keyword(s): Lithium stars - Astronomy data modeling - Chemical abundances

Status at CDS : Large table(s) will be appraised for possible ingestion in VizieR.

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 Cl Melotte 22 OpC 03 46 24.2 +24 06 50           ~ 3436 0
2 LAMOST J062739.73+463634.4 * 06 27 39.73 +46 36 34.4           ~ 1 0
3 LAMOST J093835.58-064404.6 * 09 38 35.5845564189 -06 44 04.657296828   13.100 12.347 12.223   ~ 3 0
4 2MASS J12074431+1728321 ** 12 07 44.31144 +17 28 32.1168           ~ 1 0

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