Results 191 to 200 of about 1,949,650 (217)

Line Formation in Turbulent Media

1975
Since 1934, when Struve and Elvey introduced the concept of microturbulence for spectral line broadening in addition to pressure and thermal Doppler broadening, this mechanism has frequently been used in the analysis of stellar spectra. According to the discussions in standard textbooks on stellar spectra the effect of microturbulence is due to an ...
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The First Stars: Formation, Properties, and Impact

Annual Review of Astronomy and Astrophysics, 2023
Ralf S Klessen, Simon C O Glover
exaly  

Cosmic Star-Formation History

Annual Review of Astronomy and Astrophysics, 2014
Piero Madau, Mark Dickinson
exaly  

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2000
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On the Formation of Squall Lines

Bulletin of the American Meteorological Society, 1952
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Chlorinated and brominated polycyclic aromatic hydrocarbons: Sources, formation mechanisms, and occurrence in the environment

Progress in Energy and Combustion Science, 2020
Rong Jin, Minghui Zheng, Gerhard Lammel   +2 more
exaly  

STAR FORMATION IN GALAXIES ALONG THE HUBBLE SEQUENCE

Annual Review of Astronomy and Astrophysics, 1998
Robert C Kennicutt
exaly  

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2011
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Physical Conditions in Regions of Star Formation

Annual Review of Astronomy and Astrophysics, 1999
Neal J Evans
exaly  

High-Mass Star and Massive Cluster Formation in the Milky Way

Annual Review of Astronomy and Astrophysics, 2018
F Motte, Fabien Louvet
exaly