FANG
发表于 2025-3-26 21:23:56
Introduction to Asteroseismology of , Scuti Starsere I will discuss what we can learn about the Sun by studying . Scuti stars, as well as what we can learn about stars more massive or evolved than the Sun. I will discuss some of the difficulties in theoretical approaches to asteroseismology for 8 Scuti stars, using FG Virginis, . Scuti, and CD –24° 7599 (also known as XX Pyxidis) as examples.
GORGE
发表于 2025-3-27 01:35:31
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inflame
发表于 2025-3-27 06:40:12
Techniques of Collection, Reduction and Analysis of Data of Pulsating Stars IIospheres and coronas. A detailed description is then given on how to correct photometric data for atmospheric extinction. Through a description of a “blind” statistical approach to cluster surveys we will then underline how important information about pulsating variables resides in the class more than in the individual.
doxazosin
发表于 2025-3-27 13:09:20
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Endoscope
发表于 2025-3-27 15:05:29
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frugal
发表于 2025-3-27 20:54:33
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分解
发表于 2025-3-27 21:56:11
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FEMUR
发表于 2025-3-28 03:28:37
Astrophysical Equation of State and Opacitymooth, consistent, valid over a large range of temperatures and densities, and must incorporate the most important astrophysically relevant chemical elements. The equation of state appears as a necessary part of stellar modeling as well as of any opacity calculation. For the latter, it has to provid
整理
发表于 2025-3-28 08:28:17
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exophthalmos
发表于 2025-3-28 11:55:28
The Pulsational Behaviour of Variable Stars in the Lower Part of the Instability Striphe past years a great effort was made by the stellar group of Brera Observatory (E. Antonello, M. Bossi, L. Mantegazza, E. Poretti, F.M. Zerbi) to collect a large amount of photometric and spectroscopic data on . Sct stars, the more numerous class. Observations were carried out using the telescopes