The Halo Lithium Plateau: Outstanding Issues

Sean G. Ryan; L. Elliott

doi:10.1007/978-3-540-34136-9_66

The Halo Lithium Plateau: Outstanding Issues

Sean G. Ryan
, L. Elliott

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

41 Downloads (Pure)

Abstract

We examine outstanding issues in the analysis and interpretation of the halo Li plateau. We show that the majority of very Li-poor halo Li-plateau stars (5 out of 8) have high projected rotation velocities vsini between 4.7 and 10.4 km s^-1. Such stars have very different evolutionary histories to Li-normal plateau stars, and hence cannot be included in studies of Li depletion by normal halo dwarfs. Uncertainties in the effective temperature scale for metal-poor stars continue to challenge the analysis of Li.

Original language	English
Title of host publication	Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites
Subtitle of host publication	Procs of ESO Workshop
Editors	Luca Pasquini, Sofia Randich
Publisher	Springer Nature
Pages	185-190
DOIs	https://doi.org/10.1007/978-3-540-34136-9_66
Publication status	Published - 2006
Event	ESO Workshop - Castiglione della Pescaia, Italy Duration: 13 Sept 2004 → 17 Sept 2004

Workshop

Workshop	ESO Workshop
Country/Territory	Italy
City	Castiglione della Pescaia
Period	13/09/04 → 17/09/04

Access to Document

10.1007/978-3-540-34136-9_66

901967Accepted author manuscript, 81.8 KB

Cite this

@inproceedings{77dc5b6064a54d14b80b3224345199a9,

title = "The Halo Lithium Plateau: Outstanding Issues",

abstract = "We examine outstanding issues in the analysis and interpretation of the halo Li plateau. We show that the majority of very Li-poor halo Li-plateau stars (5 out of 8) have high projected rotation velocities vsini between 4.7 and 10.4 km s-1. Such stars have very different evolutionary histories to Li-normal plateau stars, and hence cannot be included in studies of Li depletion by normal halo dwarfs. Uncertainties in the effective temperature scale for metal-poor stars continue to challenge the analysis of Li.",

author = "Ryan, \{Sean G.\} and L. Elliott",

year = "2006",

doi = "10.1007/978-3-540-34136-9\_66",

language = "English",

pages = "185--190",

editor = "Luca Pasquini and Sofia Randich",

booktitle = "Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites",

publisher = "Springer Nature ",

address = "Netherlands",

note = "ESO Workshop ; Conference date: 13-09-2004 Through 17-09-2004",

}

TY - GEN

T1 - The Halo Lithium Plateau

T2 - ESO Workshop

AU - Ryan, Sean G.

AU - Elliott, L.

PY - 2006

Y1 - 2006

N2 - We examine outstanding issues in the analysis and interpretation of the halo Li plateau. We show that the majority of very Li-poor halo Li-plateau stars (5 out of 8) have high projected rotation velocities vsini between 4.7 and 10.4 km s-1. Such stars have very different evolutionary histories to Li-normal plateau stars, and hence cannot be included in studies of Li depletion by normal halo dwarfs. Uncertainties in the effective temperature scale for metal-poor stars continue to challenge the analysis of Li.

AB - We examine outstanding issues in the analysis and interpretation of the halo Li plateau. We show that the majority of very Li-poor halo Li-plateau stars (5 out of 8) have high projected rotation velocities vsini between 4.7 and 10.4 km s-1. Such stars have very different evolutionary histories to Li-normal plateau stars, and hence cannot be included in studies of Li depletion by normal halo dwarfs. Uncertainties in the effective temperature scale for metal-poor stars continue to challenge the analysis of Li.

U2 - 10.1007/978-3-540-34136-9_66

DO - 10.1007/978-3-540-34136-9_66

M3 - Conference contribution

SP - 185

EP - 190

BT - Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites

A2 - Pasquini, Luca

A2 - Randich, Sofia

PB - Springer Nature

Y2 - 13 September 2004 through 17 September 2004

ER -

The Halo Lithium Plateau: Outstanding Issues

Abstract

Workshop

Access to Document

Fingerprint

Cite this