3D hydrodynamical model atmospheres of metal-poor stars, evidence for a low primordial Li abundance
Research output: Contribution to journal › Journal article › Research › peer-review
Standard
3D hydrodynamical model atmospheres of metal-poor stars, evidence for a low primordial Li abundance. / Asplund, M.; Nordlund, A.; Trampedach, Regner.
In: A&A Letters, No. 346, 1999, p. 17-20.Research output: Contribution to journal › Journal article › Research › peer-review
Harvard
Asplund, M, Nordlund, A & Trampedach, R 1999, '3D hydrodynamical model atmospheres of metal-poor stars, evidence for a low primordial Li abundance', A&A Letters, no. 346, pp. 17-20.
APA
Asplund, M., Nordlund, A., & Trampedach, R. (1999). 3D hydrodynamical model atmospheres of metal-poor stars, evidence for a low primordial Li abundance. A&A Letters, (346), 17-20.
Vancouver
Asplund M, Nordlund A, Trampedach R. 3D hydrodynamical model atmospheres of metal-poor stars, evidence for a low primordial Li abundance. A&A Letters. 1999;(346):17-20.
Author
Bibtex
@article{7778be7074c611dbbee902004c4f4f50,
title = "3D hydrodynamical model atmospheres of metal-poor stars, evidence for a low primordial Li abundance",
author = "M. Asplund and A. Nordlund and Regner Trampedach",
year = "1999",
language = "English",
pages = "17--20",
journal = "A&A Letters",
number = "346",
}
RIS
TY - JOUR
T1 - 3D hydrodynamical model atmospheres of metal-poor stars, evidence for a low primordial Li abundance
AU - Asplund, M.
AU - Nordlund, A.
AU - Trampedach, Regner
PY - 1999
Y1 - 1999
M3 - Journal article
SP - 17
EP - 20
JO - A&A Letters
JF - A&A Letters
IS - 346
ER -
ID: 151724