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Cited article:
N. Ryde
A&A, 455 2 (2006) L13-L16
Published online: 2006-08-04
This article has been cited by the following article(s):
13 articles
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TheGaia-ESO Survey: Galactic evolution of sulphur and zinc
S. Duffau, E. Caffau, L. Sbordone, et al. Astronomy & Astrophysics 604 A128 (2017) https://doi.org/10.1051/0004-6361/201730477
Galactic chemical evolution of sulphur
E. Matrozis, N. Ryde and A. K. Dupree Astronomy & Astrophysics 559 A115 (2013) https://doi.org/10.1051/0004-6361/201322317
Sulphur abundances in halo giants from the [S ı] line at 1082 nm and the S ı triplet around 1045 nm
H. Jönsson, N. Ryde, P. E. Nissen, et al. Astronomy & Astrophysics 530 A144 (2011) https://doi.org/10.1051/0004-6361/201116855
First stars
M. Spite, E. Caffau, S. M. Andrievsky, et al. Astronomy & Astrophysics 528 A9 (2011) https://doi.org/10.1051/0004-6361/201015926
Solar Chemical Abundances Determined with a CO5BOLD 3D Model Atmosphere
E. Caffau, H.-G. Ludwig, M. Steffen, B. Freytag and P. Bonifacio Solar Physics 268 (2) 255 (2011) https://doi.org/10.1007/s11207-010-9541-4
Sulphur abundances in halo stars from multiplet 3 at 1045 nm
E. Caffau, L. Sbordone, H.‐G. Ludwig, P. Bonifacio and M. Spite Astronomische Nachrichten 331 (7) 725 (2010) https://doi.org/10.1002/asna.201011353
Prospects of stellar abundance studies from near‐IR spectra observed with the E‐ELT
N. Ryde Astronomische Nachrichten 331 (4) 433 (2010) https://doi.org/10.1002/asna.200911345
Sulfur in the globular clusters 47 Tucanae and NGC 6752
L. Sbordone, M. Limongi, A. Chieffi, et al. Astronomy & Astrophysics 503 (1) 121 (2009) https://doi.org/10.1051/0004-6361/200811513
Stellar spectroscopy in the infrared at high spectral resolution
Nils Ryde Physica Scripta T134 014001 (2009) https://doi.org/10.1088/0031-8949/2009/T134/014001
Sulphur and zinc abundances in Galactic halo stars revisited
P. E. Nissen, C. Akerman, M. Asplund, et al. Astronomy & Astrophysics 469 (1) 319 (2007) https://doi.org/10.1051/0004-6361:20077344
The forbidden 1082 nm line of sulphur:
E. Caffau and H.-G. Ludwig Astronomy & Astrophysics 467 (1) L11 (2007) https://doi.org/10.1051/0004-6361:20077234