ANTIC
发表于 2025-3-28 17:07:25
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潜移默化
发表于 2025-3-28 21:23:02
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inferno
发表于 2025-3-29 02:19:46
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ARIA
发表于 2025-3-29 04:25:58
Three Aspects of Red Giant Studies in the Magellanic Cloudsity function carries informations about the star formation rate in the Clouds and it can be mathematically related to their history. Most AGB stars vary their magnitude in a few to several hundred years time; the one epoch DENIS magnitudes for both Large and Small Magellanic Cloud AGB stars outline the same relations as a function of period
CORE
发表于 2025-3-29 10:35:18
Structure and Evolution of AGB Stars: Current Understandings and Beyondto the formation and early evolution of our galaxy by these studies. Finally, we discuss the importance of non-standard effects in understanding the actual evolution of AGB stars and introduce some recent attempts to reveal their roles in the internal mixing and nucleosynthesis
Obverse
发表于 2025-3-29 12:15:49
Mass-Losing and Pulsating AGB Stars in the Magellanic Cloudsavailable model grid, and (3) the period-mass loss rate relation for C-rich SMC stars seems to follow that derived for Galactic carbon-rich Miras, suggesting no explicit dependence of mass loss rate on metallicity
affinity
发表于 2025-3-29 18:16:04
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种族被根除
发表于 2025-3-29 23:00:50
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Myosin
发表于 2025-3-30 01:28:05
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Irrepressible
发表于 2025-3-30 04:54:10
Photometric Properties of Long-Period Variables in the Large Magellanic Cloudtigated. Stars with large amplitudes and high periodicities were distributed on the only one strip amongst multiple structure on the LMC period-luminosity relation. In the CMD, the five strips were located in the order of the period. The stars with characterized light curves were also discussed