ke Nordlund
ke Nordlund
Professor, Niels Bohr Institute Copenhagen
Verified email at nbi.dk
TitleCited byYear
A grid of MARCS model atmospheres for late-type stars I. Methods and general properties
B Gustafsson, B Edvardsson, K Eriksson, UG Jorgensen, Nordlund, ...
Arxiv preprint arXiv:0805.0554, 2008
17792008
A grid of model atmospheres for metal-deficient giant stars. I
B Gustafsson, RA Bell, K Eriksson, Nordlund
Astronomy and Astrophysics 42, 407-432, 1975
11961975
The stellar initial mass function from turbulent fragmentation
P Padoan, Nordlund
The Astrophysical Journal 576, 870, 2002
9832002
Dynamo-generated turbulence and large-scale magnetic fields in a Keplerian shear flow
A Brandenburg, A Nordlund, RF Stein, U Torkelsson
The Astrophysical Journal 446, 741, 1995
9321995
Simulations of solar granulation. I. General properties
RF Stein, Nordlund
The Astrophysical Journal 499, 914, 1998
8701998
Line formation in solar granulation-IV.[O I], O I and OH lines and the photospheric O abundance
M Asplund, N Grevesse, AJ Sauval, CA Prieto, D Kiselman
Astronomy & Astrophysics 417 (2), 751-768, 2004
8622004
Fundamental differences between SPH and grid methods
O Agertz, B Moore, J Stadel, D Potter, F Miniati, J Read, L Mayer, ...
Monthly Notices of the Royal Astronomical Society 380 (3), 963-978, 2007
6642007
Numerical simulations of the solar granulation. I-Basic equations and methods
A Nordlund
Astronomy and Astrophysics 107, 1-10, 1982
5291982
The universality of the stellar initial mass function
P Padoan, A Nordlund, BJT Jones
Monthly Notices of the Royal Astronomical Society 288, 145-152, 1997
5181997
The universality of the stellar imf
P Padoan, A Nordlund, BJT Jones
Arxiv preprint astro-ph/9703110, 1997
518*1997
Line formation in solar granulation: I. Fe line shapes, shifts and asymmetries
M Asplund, Nordlund, R Trampedach, CA Prieto, RF Stein
Arxiv preprint astro-ph/0005320, 2000
4572000
Topology of convection beneath the solar surface
RF Stein, Nordlund
The Astrophysical Journal 342, L95-L98, 1989
4341989
The absolute chronology and thermal processing of solids in the solar protoplanetary disk
JN Connelly, M Bizzarro, AN Krot, Nordlund, D Wielandt, MA Ivanova
Science 338 (6107), 651-655, 2012
4302012
A grid of model atmospheres for metal-deficient giant stars. II
RA Bell, K Eriksson, B Gustafsson, A Nordlund
Astronomy and Astrophysics Supplement Series 23, 37-95, 1976
4261976
Solar Surface Convection. Living Rev
A Nordlund, RF Stein, M Asplund
Solar Phys 6, 2009
392*2009
A super-alfvenic model of dark clouds
P Padoan, Nordlund
The Astrophysical Journal 526, 279, 1999
3891999
" Solar Surface Convection
Nordlund, RF Stein, M Asplund
Living Reviews in Solar Physics 6 (2), 2009
3882009
Heating and activity of the solar corona 1. Boundary shearing of an initially homogeneous magnetic eld
K Galsgaard, A Nordlund
J. Geophys. Res 101, 13445-13460, 1996
3861996
Solar granulation-Influence of convection on spectral line asymmetries and wavelength shifts
D Dravins, L Lindegren, A Nordlund
Astronomy and Astrophysics 96, 345-364, 1981
3591981
Stable magnetic fields in stellar interiors
J Braithwaite, Nordlund
Astronomy & Astrophysics 450 (3), 1077-1095, 2006
3452006
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Articles 1–20