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nt of Graduate and Undergraduate Studies in Education at Brock University; his research interests include: Philosophy of education, Invitational theory and practice, Educational leadership, and Social-cultural contexts of education. .978-94-6300-214-1SHOCK 发表于 2025-3-28 23:53:51
W. Thimment of Graduate and Undergraduate Studies in Education at Brock University; his research interests include: Philosophy of education, Invitational theory and practice, Educational leadership, and Social-cultural contexts of education. .978-94-6300-214-1Malleable 发表于 2025-3-29 06:35:04
K.-P. Schürenservations of young stars and circumstellar disks and address the case of the solar system as a specific example, different from the newly discovered systems. Then the study of planetary systems and of exoplanets is presented from a more theoretical point of view. The book ends with an outlook to fuObituary 发表于 2025-3-29 08:50:11
H. Kewitzservations of young stars and circumstellar disks and address the case of the solar system as a specific example, different from the newly discovered systems. Then the study of planetary systems and of exoplanets is presented from a more theoretical point of view. The book ends with an outlook to fuALLEY 发表于 2025-3-29 11:53:12
H. Kewitzservations of young stars and circumstellar disks and address the case of the solar system as a specific example, different from the newly discovered systems. Then the study of planetary systems and of exoplanets is presented from a more theoretical point of view. The book ends with an outlook to fuDevastate 发表于 2025-3-29 18:54:38
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E. Oberdisser systems with small sepa- tions would not be favorable places for planet formation) became so strong that in a subsequent paper in 1992, Walker and his colleagues suggested that the planet in the Cephei binary might not be real, and the variations in the radial velocity of this star might have been水汽 发表于 2025-3-30 06:16:22
H.-D. Pohler systems with small sepa- tions would not be favorable places for planet formation) became so strong that in a subsequent paper in 1992, Walker and his colleagues suggested that the planet in the Cephei binary might not be real, and the variations in the radial velocity of this star might have been