无聊的人
发表于 2025-3-28 16:49:34
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无底
发表于 2025-3-28 20:07:35
Near-IR Spectroscopy and Population Synthesis of Super Star Clusters in NGC 1569ry. We fit these photospheric spectra to NextGen model atmospheres to obtain effective spectral types of clusters, and find that the information in both .- ..-band spectra is necessary to remove degeneracy in the fits. The light of SSC B is unambiguously dominated by K0 supergiants (T. = 4400 ± 100
佛刊
发表于 2025-3-29 01:26:10
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Kidnap
发表于 2025-3-29 04:59:47
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泄露
发表于 2025-3-29 11:15:36
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休战
发表于 2025-3-29 13:16:39
Starbursts Near and Far: An Overvieww high effective temperatures; 4.) determination of the initial mass function in starbursts; 5.) the nature of LINERs; and 6.) whether the huge masses deduced for the ISM in starburst regions are correct.
parsimony
发表于 2025-3-29 17:41:43
Star Formation in the Galactic Center and Nearby Nucleintly been born into massive stellar clusters. I discuss these findings and argue that the same considerations apply to most, if not all gas-rich spiral galaxies. In the mass budget of the Galactic center, star formation is apparently the dominant sink.
padding
发表于 2025-3-29 20:13:10
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来就得意
发表于 2025-3-30 02:04:55
Spectroscopy of Compact Star Clusters in NGC 4038/4039small spatial scales are seen throughout the merger. Cluster masses range from 10. to a few x 10. M.. A comparison between dynamically determined masses and those estimated from photometry in combination with starburst models suggests variations in the IMF from cluster to cluster.
Femish
发表于 2025-3-30 06:20:04
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