Occupation
发表于 2025-3-23 11:10:02
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Phagocytes
发表于 2025-3-23 17:19:13
Warm Gas at High Redshiftds and argue by comparison with cosmological simulations that Lyman . forest observations show the signs of ongoing gravitational structure formation at high redshift. The departures of observed line profiles from thermal Voigt profiles (caused by bulk motion of infalling gas and compressional heati
填料
发表于 2025-3-23 21:41:51
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OVERT
发表于 2025-3-24 00:17:50
An H I Survey of the Boötes Void those of galaxies found in a survey of regions of mean cosmic density. The Boötes survey covers 1100 Mpc., or ~ 1% of the volume of the void and consists of 24 cubes of typically 2 Mpc × 2 Mpc X 1280 km s., centered on optically known galaxies. Sixteen targets were detected in HI; 18 previously unc
canonical
发表于 2025-3-24 02:25:48
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Blatant
发表于 2025-3-24 07:24:27
Ultraluminous Infrared Galaxies: Dissipation in Forming Spheroidal Systemse.. 1991). As shown by the simulations by Barnes & Hernquist (1991), the presence of such concentrations is naturally expected in the merging of gas-rich galaxies, where the gas, being ., quickly sheds its angular momentum and sinks to the bottom of the potential well.
arboretum
发表于 2025-3-24 14:32:09
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Blood-Clot
发表于 2025-3-24 17:51:10
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谦卑
发表于 2025-3-24 20:09:01
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nugatory
发表于 2025-3-25 00:16:59
H I Imaging of Clusters of the cluster. The most distant cluster imaged in H I so far is Abell 2670 at z = 0.0767. The preliminary VLA results detect many gas rich spirals, which are exclusively located in the outer parts of the cluster. The results strengthen the suggestion (Bird 1994) that substructure is present and th