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Titlebook: Regional Opioid Analgesia; Physiopharmacologica J. Castro,J. Meynadier,M. Zenz Book 1991 Kluwer Academic Publishers 1991 Infusion.Trauma.ca

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樓主: Hermit
21#
發(fā)表于 2025-3-25 05:22:02 | 只看該作者
22#
發(fā)表于 2025-3-25 09:06:52 | 只看該作者
ck disk or halo population. Their long-lived chromospheric activity is interpreted as due to coalescence of old contact binaries. The question of the age of Proxima Centauri is examined in the context of our results, and found to be compatible with the ages of a Centauri A and B.
23#
發(fā)表于 2025-3-25 15:12:15 | 只看該作者
24#
發(fā)表于 2025-3-25 18:32:14 | 只看該作者
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.ck disk or halo population. Their long-lived chromospheric activity is interpreted as due to coalescence of old contact binaries. The question of the age of Proxima Centauri is examined in the context of our results, and found to be compatible with the ages of a Centauri A and B.
25#
發(fā)表于 2025-3-25 23:33:43 | 只看該作者
26#
發(fā)表于 2025-3-26 00:18:26 | 只看該作者
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.ck disk or halo population. Their long-lived chromospheric activity is interpreted as due to coalescence of old contact binaries. The question of the age of Proxima Centauri is examined in the context of our results, and found to be compatible with the ages of a Centauri A and B.
27#
發(fā)表于 2025-3-26 05:23:43 | 只看該作者
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.ck disk or halo population. Their long-lived chromospheric activity is interpreted as due to coalescence of old contact binaries. The question of the age of Proxima Centauri is examined in the context of our results, and found to be compatible with the ages of a Centauri A and B.
28#
發(fā)表于 2025-3-26 12:04:58 | 只看該作者
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.ck disk or halo population. Their long-lived chromospheric activity is interpreted as due to coalescence of old contact binaries. The question of the age of Proxima Centauri is examined in the context of our results, and found to be compatible with the ages of a Centauri A and B.
29#
發(fā)表于 2025-3-26 13:28:08 | 只看該作者
30#
發(fā)表于 2025-3-26 20:01:54 | 只看該作者
J. De Castro M.D.,J. Meynadier M.D.,M. Zenz M.D.ck disk or halo population. Their long-lived chromospheric activity is interpreted as due to coalescence of old contact binaries. The question of the age of Proxima Centauri is examined in the context of our results, and found to be compatible with the ages of a Centauri A and B.
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