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Titlebook: Cosmic Chemistry; Gerhard Klare Conference proceedings 1988 Springer-Verlag Berlin Heidelberg 1988 astrophysics.galaxies.interstellar matt

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樓主: EFFCT
31#
發(fā)表于 2025-3-26 22:26:01 | 只看該作者
32#
發(fā)表于 2025-3-27 05:09:41 | 只看該作者
33#
發(fā)表于 2025-3-27 08:49:31 | 只看該作者
34#
發(fā)表于 2025-3-27 09:43:57 | 只看該作者
0941-1445 astrophysics. The twelve contributions to this book, written by experts from the US, UK, France, Belgium, Switzerland and Germany, deal in depth with the chemistry of comets and meteorites, of stars and their shells, of the interstellar medium and galaxies. A comprehensive review of nucleosynthesis
35#
發(fā)表于 2025-3-27 16:02:39 | 只看該作者
Vertical Profiles Over Flat Terrain,, were used to sample about 7700 deg. with the angular resolution degraded to 0.5° in order to cover large areas quickly. Other surveys used significantly higher angular resolution but have been limited to selected nearby molecular clouds and a thin strip covering the inner galactic plane. The most extensive of these surveys are:
36#
發(fā)表于 2025-3-27 18:52:21 | 只看該作者
37#
發(fā)表于 2025-3-28 01:29:34 | 只看該作者
38#
發(fā)表于 2025-3-28 02:07:06 | 只看該作者
Vertical Profiles Over Flat Terrain, ≈ 82 and 50 neighbours, may be sufficient to explain the observed r-abundances in the A ≈ 130 and 80 abundance peaks. Based on this result, new constraints are given on the stellar conditions under which a steady-flow r-process has operated.
39#
發(fā)表于 2025-3-28 08:47:45 | 只看該作者
40#
發(fā)表于 2025-3-28 13:34:17 | 只看該作者
,Nuclear Physics Constraints to Bring the Astrophysical R-Process to the “Waiting Point”, ≈ 82 and 50 neighbours, may be sufficient to explain the observed r-abundances in the A ≈ 130 and 80 abundance peaks. Based on this result, new constraints are given on the stellar conditions under which a steady-flow r-process has operated.
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