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┼ke Nordlund
┼ke Nordlund
Professor, Niels Bohr Institute Copenhagen
Verified email at nbi.dk
Title
Cited by
Cited by
Year
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
27562008
A grid of model atmospheres for metal-deficient giant stars. I
B Gustafsson, RA Bell, K Eriksson, ┼ Nordlund
Astronomy and Astrophysics, vol. 42, no. 3, Sept. 1975, p. 407-432. Researchá…, 1975
13061975
The stellar initial mass function from turbulent fragmentation
P Padoan, ┼ Nordlund
The Astrophysical Journal 576, 870, 2002
12122002
Dynamo-generated turbulence and large-scale magnetic fields in a Keplerian shear flow
A Brandenburg, A Nordlund, RF Stein, U Torkelsson
Astrophysical Journal v. 446, p. 741 446, 741, 1995
10531995
Simulations of solar granulation. I. General properties
RF Stein, ┼ Nordlund
The Astrophysical Journal 499, 914, 1998
10041998
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
8352007
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
7762012
The universality of the stellar imf
P Padoan, A Nordlund, BJT Jones
Arxiv preprint astro-ph/9703110, 1997
619*1997
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
6171997
Numerical simulations of the solar granulation. I-Basic equations and methods
A Nordlund
Astronomy and Astrophysics, vol. 107, no. 1, Mar. 1982, p. 1-10. Researchá…, 1982
5951982
Solar Surface Convection. Living Rev
A Nordlund, RF Stein, M Asplund
Solar Phys 6, 2009
564*2009
" Solar Surface Convection
┼ Nordlund, RF Stein, M Asplund
Living Reviews in Solar Physics 6 (2), 2009
5572009
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
5162000
The Star Formation Rate of Supersonic Magnetohydrodynamic Turbulence
P Padoan, ┼ Nordlund
The Astrophysical Journal 730, 40, 2011
5112011
A grid of model atmospheres for metal-deficient giant stars. II
RA Bell, K Eriksson, B Gustafsson, A Nordlund
Astronomy and Astrophysics Supplement Series, vol. 23, Jan. 1976, p. 37-95á…, 1976
5021976
A super-alfvenic model of dark clouds
P Padoan, ┼ Nordlund
The Astrophysical Journal 526, 279, 1999
4581999
Topology of convection beneath the solar surface
RF Stein, ┼ Nordlund
Astrophysical Journal, Part 2-Letters (ISSN 0004-637X), vol. 342, July 15á…, 1989
4531989
Solar granulation-Influence of convection on spectral line asymmetries and wavelength shifts
D Dravins, L Lindegren, A Nordlund
Astronomy and Astrophysics, vol. 96, no. 1-2, Mar. 1981, p. 345-364á…, 1981
4431981
Stable magnetic fields in stellar interiors
J Braithwaite, ┼ Nordlund
Astronomy & Astrophysics 450 (3), 1077-1095, 2006
4312006
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
4311996
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Articles 1–20