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Massive Stars: Input Physics and Stellar Models.

• Authors : EI Eid, M. F.¹ ; The, L.-S.² ; Meyer, B. S.²

• Source: Space Science Reviews. Apr2009, Vol. 147 Issue 1/2, p1-29. 29p. 5 Charts, 10 Graphs.

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SOLIDS IN SPACE.

• Authors : Henning, Thomas K.

• Source: Science Spectra. 2000, Issue 23, p56. 8p. 5 Color Photographs, 2 Black and White Photographs, 3 Diagrams, 1 Chart, 3 Graphs.

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An intensity map of hydrogen 21-cm emission at redshift z ≈ 0.8.

• Authors : Tzu-Ching Chang^1,2 ; Ue-Li Pen²; Bandura, Kevin³

Subjects: *METAPHYSICAL cosmology; *REDSHIFT; *HYDROGEN

• Source: Nature. 7/22/2010, Vol. 466 Issue 7305, p463-465. 3p. 2 Graphs.

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Radioactive 26Al from massive stars in the Galaxy.

• Authors : Diehl, Roland¹; Halloin, Hubert¹; Kretschmer, Karsten¹

Subjects: *GAMMA rays; *SUPERGIANT stars; *GALAXIES

• Source: Nature. 1/5/2006, Vol. 439 Issue 7072, p45-47. 3p. 1 Graph.

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The elemental abundance pattern in a galaxy at z = 2.626.

• Authors : Prochaska, Jason X.; Howk, J. Christopher; Wolfe, Arthur M.

Subjects: *COSMIC abundances; *COSMOCHEMISTRY; *GALAXIES

• Source: Nature. 5/1/2003, Vol. 423 Issue 6935, p57. 3p.

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Applications of abundance data and requirements for cosmochemical modeling

• Authors : Wiens, R [Roger C.]

• Source: Conference: "Submitted to: Proceedings of the Joint SOHO-ACE Workshop on Solar Galactic Composition"

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Model for GCR-particle fluxes in stony meteorites and production rates of cosmogenic nuclides

• Authors : Reedy, R

• Source: Conference: 15. lunar and planetary science conference, Houston, TX, USA, 12 Mar 1984; Other Information: Portions are illegible in microfiche products

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Rubidium-Rich Asymptotic Giant Branch Stars.

• Authors : García-Hernández, D. A.; García-Lario, P.; Plez, B.

Subjects: ASYMPTOTIC giant branch stars; NUCLEOSYNTHESIS; DEBATE

• Source: Science. 12/15/2006, Vol. 314 Issue 5806, p1751-1754. 5p.

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(Astrophysics of binary stars, Seyfert galaxies, quasars, and globular clusters. Final technical report

• Authors : Press, W

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Nuclear chemistry and geochemistry research. Progress report, 1973--1976

• Authors : Kohman, T

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