DRILL
发表于 2025-3-23 13:30:18
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不可比拟
发表于 2025-3-23 16:37:49
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faultfinder
发表于 2025-3-23 21:09:48
a in the gastrointestinal system.Resource on direct-fed micr.The practice of supplementing direct fed microbial and prebiotic additives to domestic animals during growth is becoming more widespread in food animal production. Beneficial effects particularly in cattle, pigs and poultry, including imp
易改变
发表于 2025-3-24 00:17:22
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verdict
发表于 2025-3-24 03:27:18
https://doi.org/10.1057/978-1-137-51911-5Since the time of .., the appearance of protein in the urine has been associated with the presence of renal disease.
蚊帐
发表于 2025-3-24 08:14:15
Mitgliederversammlung (Zweiter Teil): Meine sehr verehrten Damen und Herren, liebe Kolleginnen und Kollegen! Ich eröffne die Mitgliederversammlung Teil II, und begrüße Sie sehr herzlich.
cajole
发表于 2025-3-24 14:00:36
Concepts for Reforming the Political SystemProminently displayed in each meeting room was the stated purpose of this Dahlem Conference: .. We were inquiring whether nonhuman animals have mental experiences, and if so which animals, under what conditions.
Narcissist
发表于 2025-3-24 17:36:43
https://doi.org/10.1057/9781403920218The rotational properties of pre-main sequence stars with a mass between 0.5 and 9 M. are reviewed. The impact of binarity and disk accretion upon early rotational evolution is discussed and unsolved problems related to the evolution of stellar angular momentum prior to the main sequence are outlined.
escalate
发表于 2025-3-24 21:29:13
Ehrungen und PreisverleihungenIch glaube sagen zu können, unsere Gesellschaft ehrt sich in besonderer Weise selbst durch die Ernennung herausragender Persönlichkeiten zu ihren Ehrenmitgliedern. Ich darf Frau Prof. Dr. Ursula Schmidt-Tintemann, Herrn Prof. Dr. Lassalle Leffall und Herrn Prof. Dr. Alexander Fjodorowitsch Chernousov auf die Bühne bitten.
Obsequious
发表于 2025-3-25 01:02:02
Robert David Cruz,Maria J. WillumsenThe properties of young stars of intermediate—mass are discussed in the light of recent calculations of the protostellar accretion phase. In particular, the problem of the existence of surface convection in these stars will be addressed with reference to the strong activity manifested by the Herbig Ae/Be stars.