成绩上升
发表于 2025-3-30 09:29:03
Infrared Astronomy with Arrays978-94-011-1070-9Series ISSN 0067-0057 Series E-ISSN 2214-7985
Migratory
发表于 2025-3-30 15:31:56
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CYN
发表于 2025-3-30 20:23:01
The Mass Function of Faint Field Galaxiese consistent with the no-evolution or pure luminosity evolution models. The excess faint blue galaxies seen in the B band number counts at intermediate magnitudes are a result of a low normalization, and do not dominate the population until . ≈ 25. Extreme merging or excess dwarf models are not needed.
施舍
发表于 2025-3-30 22:31:38
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optional
发表于 2025-3-31 03:03:44
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pus840
发表于 2025-3-31 06:24:00
Application of Near-IR Spectroscopy to the Study of the Stellar Content in Starburst Galaxiesd metallicity and ellipticals). Using proper IR spectral indices, which have been found to be powerful indicators of temperature in cool stars, some preliminary consideration on the dominant stellar population in the nuclear region of these galaxies are drawn.
Melatonin
发表于 2025-3-31 12:21:06
Astrophysics and Space Science Libraryhttp://image.papertrans.cn/i/image/466267.jpg
乳白光
发表于 2025-3-31 15:06:13
Book 1994 of the Hilo conference, excitement was running high and everyone present was in favor of another meeting. I recall suggesting to Al Fowler that the next meeting could be in Tucson. Despite Al‘s reply to the effect that Hawaii was a much nicer location, a meeting was held in Tucson three years later
intuition
发表于 2025-3-31 19:10:52
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MILL
发表于 2025-3-31 23:13:26
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