Titlebook: Cool Stars with Excesses of Heavy Elements; Proceedings of the S Mercedes Jaschek,Philip C. Keenan Conference proceedings 1985 D. Reidel Pu

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Cool Stars with Excesses of Heavy Elements978-94-009-5325-3Series ISSN 0067-0057 Series E-ISSN 2214-7985

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Reliability Improvement Warranties,e spectra we examine the more evident it becomes that the groups that we are talking about here are practically never discrete and clearly bounded. There always seem to be marginal stars that blur the distinctions between the so-called groups.

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Springer Series in Reliability Engineeringconnection with the identification of .CN, .CN, HCN, [CI] λ8727, and telluric H.O lines. The microphotometric tracing of the same region of an M-type star μ Cep seems very helpful for the identification of telluric H.O lines.

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Reliability Improvement Warranties,ristics of H.D. barium-star suspects south of δ = -26ΰ found on moderate-dispersion objective-prism plates. For stars of the type that can be found from such plates, the frequency appears to lie between one-half and one percent.

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https://doi.org/10.1007/978-94-009-5325-3Galaxy; LOPES; Libration; earth; galaxies; observatory; photometry; planet; star; stars; stellar; stellar evolu

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