Results 181 to 190 of about 2,291 (216)
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Physics Bulletin, 1959
By Zdeněk Kopal London : Chapman and Hall Ltd. Pp. xiv + 558. Price 105s. At first sight this work, on the relationship between pairs of stars evolving in such close association as to be almost in contact, might appear so specialized as not to attract many general physicists.
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By Zdeněk Kopal London : Chapman and Hall Ltd. Pp. xiv + 558. Price 105s. At first sight this work, on the relationship between pairs of stars evolving in such close association as to be almost in contact, might appear so specialized as not to attract many general physicists.
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Close contact behaviors of university and school students in 10 indoor environments
Journal of Hazardous Materials, 2023Zhiyang Dou, Jianjian Wei
exaly
1990
Since the 1970s symposia or colloquia devoted to recent research on close binaries have been held around the world almost annually. At meetings of the General Assembly of the International Astronomical Union this topic has also been discussed in detail at presentations in various commission meetings and also as invited talks by leading astronomers in ...
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Since the 1970s symposia or colloquia devoted to recent research on close binaries have been held around the world almost annually. At meetings of the General Assembly of the International Astronomical Union this topic has also been discussed in detail at presentations in various commission meetings and also as invited talks by leading astronomers in ...
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Understanding and managing identification uncertainty of close modes in operational modal analysis
Mechanical Systems and Signal Processing, 2021Siu-Kui Au +2 more
exaly
Close contact behavior-based COVID-19 transmission and interventions in a subway system
Journal of Hazardous Materials, 2022Zhiyang Dou, Jianjian Wei, Nan Zhang
exaly
Close contact behavior in indoor environment and transmission of respiratory infection
Indoor Air, 2020Nan Zhang, Pak-To Chan, Hui-Ling Yen
exaly
2018
Context. Massive stars with solar metallicity lose important amounts of rotational angular momentum through their winds. When a magnetic field is present at the surface of a star, efficient angular momentum losses can still be achieved even when the mass-loss rate is very modest, at lower metallicities, or for lower-initial-mass stars.
Song, H.F. +10 more
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Context. Massive stars with solar metallicity lose important amounts of rotational angular momentum through their winds. When a magnetic field is present at the surface of a star, efficient angular momentum losses can still be achieved even when the mass-loss rate is very modest, at lower metallicities, or for lower-initial-mass stars.
Song, H.F. +10 more
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Enhancing H2 Uptake by “Close‐Packing” Alignment of Open Copper Sites in Metal–Organic Frameworks
Angewandte Chemie - International Edition, 2008Shengqian Ma +2 more
exaly