食草 发表于 2025-3-25 05:40:06
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Age and Processes of Star Formation in Very Young LMC Associationsor extragalactic HII regions and associations in the neighboring galaxies..Theoretical time evolution models of the UV-flux, the number of Lyman continuum photons, the effective temperature of the exciting stars and of the equivalent width of Hβ have been computed for three star formation rates (bur卜闻 发表于 2025-3-26 01:41:54
On the Relationship between Neutral Hydrogen Mass, Luminosity and Color in Irregular Galaxiese or low surface brightness. This is not valid for active bright irregulars of the Markaryan class. Active star-forming galaxies are segregated from quiescent ones in an (U-V) versus (log M./L) plot. This diagram can be interpreted as an evolutionary diagram if we suppose that the stellar formationmighty 发表于 2025-3-26 08:18:37
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Galaxy Encounters and the Holmberg Effectons which substantially alter a galaxy’s morphology are relatively common. Continuing effects of the encounters on the star formation rate may be revealing themselves in the ., which is a strong color correlation and coupling of apparent Hubble types found among binary galaxies.Conscientious 发表于 2025-3-26 18:19:45
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