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Results 1 to 25 of 738

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The elemental abundance pattern in a galaxy at z = 2.626PROCHASKA, Jason X; HOWK, J. Christopher; WOLFE, Arthur M et al.Nature (London). 2003, Vol 423, Num 6935, pp 57-59, issn 0028-0836, 3 p.Article

Atmospheric elemental abundances for the components of the multiple system ADS 11061. 41 draconisBALEGA, Yu. Yu; LEUSHIN, V. V; WEIGELT, G et al.Astronomy reports. 2005, Vol 49, Num 3, pp 217-225, issn 1063-7729, 9 p.Article

Evolution of elemental abundances in planetary nebulaeMILANOVA, Yu. V; KHOLTYGIN, A. F; SAMUS, N et al.Astronomy letters (Print). 2006, Vol 32, Num 8, pp 557-565, issn 1063-7737, 9 p.Article

Taking Another Look : Light n-Capture Element Abundances in Metal-Poor Halo StarsBURRIS, D; LUSK, J; JONES, E. M et al.Publications of the Astronomical Society of the Pacific. 2009, Vol 121, Num 876, pp 111-116, issn 0004-6280, 6 p.Article

The homogeneity of interstellar elemental abundances in the galactic diskCARTLEDGE, Stefan I. B; LAUROESCH, J. T; MEYER, David M et al.The Astrophysical journal. 2006, Vol 641, Num 1, pp 327-346, issn 0004-637X, 20 p., 1Article

Diffusion des éléments légers et importance de la rotation dans le soleil et les étoiles: Comparaison avec les résultats de l'héliosismologie = Diffusion of light elements and importance of rotation in the sun and the stars: Comparison with heliosismological resultsGaige, Yves; Vauclair, S.1994, 120 p.Thesis

Chemical abundance behavior of type I planetary nebulaeFAUNDEZ-ABANS, M; JIMENEZ O., J. L.Astrophysics and space science. 1993, Vol 207, Num 1, pp 47-53, issn 0004-640XArticle

Using solar p-modes to determine the convection zone depth and constrain diffusion-produced composition gradientsGUZIK, J. A; COX, A. N.The Astrophysical journal. 1993, Vol 411, Num 1, pp 394-401, issn 0004-637X, 1Article

What is new about the new comet Yanaka (1988r) ?GREENBERG, J. M; SINGH, P. D; DE ALMEIDA, A. A et al.The Astrophysical journal. 1993, Vol 414, Num 1, pp L45-L48, issn 0004-637X, 2Article

Temperature behavior of elemental abundances in the atmospheres of magnetic peculiar starsRYABCHIKOVA, T. A; SAMUS, N.Astronomy letters (Print). 2005, Vol 31, Num 6, pp 388-397, issn 1063-7737, 10 p.Article

Role of isotope mass spectrometry in cosmic abundance studiesDE LAETER, J. R.Mass spectrometry reviews (Print). 1994, Vol 13, Num 1, pp 3-22, issn 0277-7037Article

A compiled catalog of spectroscopically determined elemental abundances for stars with accurate parallaxes; magnesiumBORKOVA, T. V; MARSAKOV, V. A.Astronomy reports. 2005, Vol 49, Num 5, pp 405-416, issn 1063-7729, 12 p.Article

Laboratory simulations of Mars aqueous geochemistryBULLOCK, Mark A; MOORE, Jeffrey M; MELLON, Michael T et al.Icarus (New York, NY). 2004, Vol 170, Num 2, pp 404-423, issn 0019-1035, 20 p.Article

Evidence for a dispersion in the lithium abundances of extreme halo starsDELIYANNIS, C. P; PINSONNEAULT, M. H; DUNCAN, D. K et al.The Astrophysical journal. 1993, Vol 414, Num 2, pp 740-758, issn 0004-637X, 1Article

Jupiter formed with more tar than iceLODDERS, Katharina.The Astrophysical journal. 2004, Vol 611, Num 1, pp 587-597, issn 0004-637X, 11 p., 1Article

Estimation of (Cl-Mn)/Fe flux ratio at relativistic energies using steady-state leaky-box model modified for reaccelerationsMAJUMDAR, R; BASU, B; BHATTACHARYYA, D. P et al.Nuovo cimento della società italiana di fisica. C. 1997, Vol 20, Num 4, pp 491-496, issn 0390-5551Article

The nature of the molecular cores in high-latitude cirrus clouds. IV: The electron distribution and the abundance and chemistry of H2COTURNER, B. E.The Astrophysical journal. 1993, Vol 410, Num 1, pp 140-156, issn 0004-637X, 1Article

The r- and s-Process Contributions to Heavy-Element Abundances in the Halo Star HD 29907SITNOVA, T. M; MASHONKINA, L. I; ASTAKHOV, V et al.Astronomy letters (Print). 2011, Vol 37, Num 7, pp 480-498, issn 1063-7737, 19 p.Article

Comparison of distributed reacceleration and leaky-box models of cosmic-ray abundances (3 ≤ Z ≤ 28)LETAW, J. R; SILBERBERG, R; TSAO, C. H et al.The Astrophysical journal. 1993, Vol 414, Num 2, pp 601-611, issn 0004-637X, 1Article

Galactic cepheids. I. Elemental abundances and their implementation for stellar and galactic evolutionKOVTYUKH, V. V; WALLERSTEIN, G; ANDRIEVSKY, S. M et al.Publications of the Astronomical Society of the Pacific. 2005, Vol 117, Num 837, pp 1173-1181, issn 0004-6280, 9 p.Article

A study of circumstellar envelopes around bright carbon stars. II: Molecular abundancesOLOFSSON, H; ERIKSSON, K; GUSTAFSSON, B et al.The Astrophysical journal. Supplement series. 1993, Vol 87, Num 1, pp 305-330, issn 0067-0049Article

Error Analysis of Light n-Capture Element Abundances in the Metal-Poor Halo Star HD74462LUSK, Jeremy A; BURRIS, Debra L.Publications of the Astronomical Society of the Pacific. 2011, Vol 123, Num 901, pp 253-258, issn 0004-6280, 6 p.Article

Variations on solar condensation : Sources of interstellar dust nucleiEBEL, D. S.Journal of geophysical research. 2000, Vol 105, Num A5, pp 10363-10370, issn 0148-0227Article

Effects of the redistribution of water in the solar nebula on nebular chemistryCYR, K. E; SHARP, C. M; LUNINE, J. L et al.Journal of geophysical research. 1999, Vol 104, Num E8, pp 19003-19014, issn 0148-0227Article

Astration of deuterium during the evolution of the solar neighbourhoodRANA, N. C; KOUSALYA, P.Astrophysics and space science. 1993, Vol 207, Num 1, pp 129-132, issn 0004-640XArticle

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