Line formation in solar granulation, II. The photospheric Fe abundance
Research output: Contribution to journal › Journal article › Research › peer-review
Standard
Line formation in solar granulation, II. The photospheric Fe abundance. / Asplund, M.; Nordlund, A.; Trampedach, Regner; Stein, R.F.
In: Astronomy & Astrophysics, No. 359, 2000, p. 743-754.Research output: Contribution to journal › Journal article › Research › peer-review
Harvard
Asplund, M, Nordlund, A, Trampedach, R & Stein, RF 2000, 'Line formation in solar granulation, II. The photospheric Fe abundance', Astronomy & Astrophysics, no. 359, pp. 743-754.
APA
Asplund, M., Nordlund, A., Trampedach, R., & Stein, R. F. (2000). Line formation in solar granulation, II. The photospheric Fe abundance. Astronomy & Astrophysics, (359), 743-754.
Vancouver
Asplund M, Nordlund A, Trampedach R, Stein RF. Line formation in solar granulation, II. The photospheric Fe abundance. Astronomy & Astrophysics. 2000;(359):743-754.
Author
Bibtex
@article{329a480074c611dbbee902004c4f4f50,
title = "Line formation in solar granulation, II. The photospheric Fe abundance",
author = "M. Asplund and A. Nordlund and Regner Trampedach and R.F. Stein",
year = "2000",
language = "English",
pages = "743--754",
journal = "Astronomy & Astrophysics",
issn = "0004-6361",
publisher = "E D P Sciences",
number = "359",
}
RIS
TY - JOUR
T1 - Line formation in solar granulation, II. The photospheric Fe abundance
AU - Asplund, M.
AU - Nordlund, A.
AU - Trampedach, Regner
AU - Stein, R.F.
PY - 2000
Y1 - 2000
M3 - Journal article
SP - 743
EP - 754
JO - Astronomy & Astrophysics
JF - Astronomy & Astrophysics
SN - 0004-6361
IS - 359
ER -
ID: 147567