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Titlebook: Dynamics and Interactions of Galaxies; Proceedings of the I Roland Wielen Conference proceedings 1990 Springer-Verlag Berlin Heidelberg 199

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發(fā)表于 2025-3-30 10:45:19 | 只看該作者
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發(fā)表于 2025-3-30 15:29:01 | 只看該作者
Eustáquio J. Reis,Fernando A. Blanconation of globular cluster ages, and has allowed at least relative ages to be derived with a new level of precision. Despite controversy over many of the details, agreement is beginning to emerge that some very significant age differences do exist among globular clusters.
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發(fā)表于 2025-3-30 16:58:28 | 只看該作者
Eustáquio J. Reis,Fernando A. Blancok galaxies may have formed through mergers. As we shall see, it now seems likely that the present position of a galaxy in Hubble’s morphological sequence was determined mainly by the number and severity of mergers in its past history.
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發(fā)表于 2025-3-30 22:58:58 | 只看該作者
Are Our Globular Clusters Coeval?nation of globular cluster ages, and has allowed at least relative ages to be derived with a new level of precision. Despite controversy over many of the details, agreement is beginning to emerge that some very significant age differences do exist among globular clusters.
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