dialect
发表于 2025-3-25 03:40:26
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FECK
发表于 2025-3-25 11:24:06
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笨重
发表于 2025-3-25 14:28:13
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panorama
发表于 2025-3-25 18:14:32
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Pageant
发表于 2025-3-25 22:11:34
ISO Observations of Pre-Stellar Cores and Young Stellar Objectsples of sources in different evolutionary stages are reviewed, addressing in particular how the physical and chemical properties of the proto-stellar environments change from the pre-stellar cores to the protostars at the end of their accretion phase. In addition, the mid-IR surveys in nearby star-f
perjury
发表于 2025-3-26 03:16:30
Pre-Main Sequence Stars Seen by ISObservatory (ISO) are reviewed. All the observations have been mainly carried out by using the two spectrographs SWS and LWS, adopting their low resolution modes and such data have been used both for lines detection and to reconstruct the spectral energy distributions. Line emission and photometric b
OGLE
发表于 2025-3-26 06:42:21
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Cholagogue
发表于 2025-3-26 08:46:15
Late Stages of Stellar Evolutiontalline silicates and the rotational lines of water vapour, were detected for the first time in the spectra of (post-)Asymptotic Giant Branch (AGB) stars. Their analysis has greatly improved our knowledge of stellar atmospheres and circumstellar environments. A surprising number of objects, particul
偏狂症
发表于 2025-3-26 16:22:46
The Cool Interstellar Mediumrstanding of the physics and chemistry of the gas, the nature and evolution of the dust grains and also the coupling between the gas and the grains. We review here the ISO results on the cool and low-excitation regions of the interstellar medium, where . .≲ 500 K, .H ∼ 100–10. cm. and the electron d
浮雕宝石
发表于 2025-3-26 19:34:51
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