激励
发表于 2025-3-28 16:35:20
Photometric and Spectrophotometric Models in the NIRsed. One is a refined spectral synthesis of starbursts in the . band. Another model aims to predict synthetic spectra (continua and lines) and colors of starbursts and the Hubble Sequence from 220Å to 5μm.
国家明智
发表于 2025-3-28 19:11:02
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踉跄
发表于 2025-3-29 00:58:18
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装饰
发表于 2025-3-29 05:26:07
Colour Gradients in the Optical and Near-IRroadband colours are easy to obtain for large samples of objects, making them ideal for statistical studies. In this paper I use the radial distribution of the colours in galaxies, which gives more insight into the local processes driving the global colour differences than integrated colours. Almost
衰弱的心
发表于 2025-3-29 08:31:02
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脱水
发表于 2025-3-29 14:04:56
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Alopecia-Areata
发表于 2025-3-29 18:13:22
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jagged
发表于 2025-3-29 23:10:57
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defile
发表于 2025-3-30 00:52:52
Imaging of Local Group Bulge Populations in the Near Infrarede from a globular cluster-aged stellar population. Giants with .. < -5 are found in M31, M32, and M33, and the HST imaging strongly supports the idea that ground-based observers are not being confused by blended images of stars. On the other hand, a direct measurement of the age of the Galactic bulg
惰性女人
发表于 2025-3-30 04:06:26
Origin of Bulgesart of the spheroid formation process, that includes halo and bulge. In a more recently proposed scenario bulges form late, as a result of the dynamical evolution of a disk that is prone to develop a bar instability. Recent . and . results are reported that may help chosing among these two alternati