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Abstract (A&A 432 p.L21)
References of A&A 432 p. L21
- Bagnulo, S., Jehin, E., Ledoux, C., et al., & the ESO Paranal Science Operations Team 2004, http://www.sc.eso.org/santiago/uvespop/ (see also ESO Messenger, 114, 10, 2003)
- Bohlender, D. A., Bolduc-Duval, J., Sigut, A., & Landstreet, J. D. 2003, in Modelling of Stellar Atmospheres, ed. N. Piskunov, W. W. Weiss, & D. F. Gray, IAU Symp., 210, 426 (D3)
- Brault, J. W., & White, O. R. 1971, A&A, 13, 169 [NASA ADS]
- Castelli, F., & Hubrig, S. 2004, A&A, 421, L1 [EDP Sciences] [NASA ADS] [CrossRef]
- Clayton, D. D. 2003, Handbook of isotopes in the cosmos-hydrogen to gallium (Cambridge Univ. Press)
- Cowan, R. D. 1981, The Theory of Atomic Structure and Spectra (Berkeley: Univ. Calif. Press), 506
- Cowley, C. R., & Hensberge, H. 1981, ApJ, 244, 252 [NASA ADS] [CrossRef]
- Cowley, C. R., Hubrig, S., Ryabchikova, T. A., et al. 2001, A&A, 367, 939 [EDP Sciences] [NASA ADS] [CrossRef]
- Hinkle, K. H., Wallace, L., & Livingston, W. 1995, in Laboratory and Astronomical High Resolution Spectra, ed. A. J. Sauval, R. Blomme, & N. Grevesse, ASP Conf. Ser., 81, 66
- Hubrig, S., Kurtz, D. W., Bagnulo, S., et al. 2004a, A&A, 415, 661 [EDP Sciences] [NASA ADS] [CrossRef]
- Hubrig, S., Szeifert, T., Schöller, M., et al. 2004b, A&A, 415, 685 [EDP Sciences] [NASA ADS] [CrossRef]
- Katz, D., Munari, U., Cropper, M., et al. 2004, MNRAS, 354, 1223 [NASA ADS] [CrossRef]
- Kurtz, D. W. 1990, A&A, 423, 705 [EDP Sciences]
- Leone, F., & Catanzaro, G. 2004, A&A, 425, 271 [EDP Sciences] [NASA ADS] [CrossRef]
- Leone, F., Vacca, W. D., & Stift, M. J. 2003, A&A, 409, 1055 [EDP Sciences] [NASA ADS] [CrossRef]
- Mathys, G., Hubrig, S., Landstreet, J. D., et al. 1997, A&AS, 133, 353 [NASA ADS]
- Moore, C. E., Minnaert, M. G. J., & Houtgast, J. 1966, The Solar Spectrum 2935 Å to 8770 Å, NBS Monog., 61
- Nörtershäuser, W., Blaum, K., Icker, P., et al. 1998, Eur. Phys. J. D, 2, 33 [EDP Sciences] [NASA ADS]
- Proffitt, C. R., Brage, T., Leckrone, D. S., et al. 1999, ApJ, 512, 942 [NASA ADS] [CrossRef]
- Renson, P., Girbaldi, M., & Catalano, F. M. 1991, A&AS, 89 429
- Ryabchikova, T., Nesvacil, N., Weiss, W. W., et al. 2004, A&A, 423, 705 [EDP Sciences] [NASA ADS] [CrossRef]
- Sansonetti, J. E., & Martin, W. F. 2003, Handbook of Basic Atomic Spectroscopic Data, http://physics.nist.gov/PhysRefData/Handbook/index.html
- Wallace, L., Livingston, W. C., Bernath, P. F., & Ram, R. S. 1998, An Atlas of the Sunspot Umbral Spectrum in the Red and Infrared from 8900 to 15 050 cm-1 (6642 to 11 230 Å)
Abstract (A&A 432 p.L21)
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