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The Structure and Rotation of the Galaxy
Publications of the Astronomical Society of the Pacific, 1932For uncounted generations thoughtful men, philosophers and mathematicians, physicists and astronomers, as well as many other students, have been puzzling over the nature of our surroundings in space. They have not been satisfied, as I am afraid many of us are satisfied, with their merely terrestrial surroundings but have tiied to penetrate the almost ...
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The Structure of Elliptical Galaxies
1988Recent imaging investigations highlight the structural diversity of elliptical galaxies. The distribution of light within the cores and envelopes shows a wide range in central and average system stellar densities at any galaxy luminosity. These variations appear to offer new information on galaxy formation mechanisms.
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The structure of elliptical galaxies and galaxy clusters
1995Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 1995. ; Includes bibliographical references. ; by David Augustin Buote. ; Ph.D.
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STRUCTURE AND EVOLUTION OF CLUSTER GALAXIES
Thinking, Observing and Mining the Universe, 2004Busarello G +5 more
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Structure and Evolution of the Galaxy
1971The present volume contains papers presented during the Advanced Study Institute on the 'Structure and Evolution of the Galaxy' held under the auspices of the Science Committee, North Atlantic Treaty Organization (NATO) in Lagonissi near Athens, Greece between 8-19 September 1969.
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A Journey from Structure to Function of Bacterial Lipopolysaccharides
Chemical Reviews, 2022Katarzyna Duda +2 more
exaly
2005
Tracing the spiral structure of our Galaxy requires to identify and position the star-forming complexes. Each complex can be seen as a parental molecular cloud with associated ionised hydrogen, young stars and young clusters. The analysis of the ionised gas at Halpha wavelength (diffuse emission as well as discrete HII regions) is essential to ...
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Tracing the spiral structure of our Galaxy requires to identify and position the star-forming complexes. Each complex can be seen as a parental molecular cloud with associated ionised hydrogen, young stars and young clusters. The analysis of the ionised gas at Halpha wavelength (diffuse emission as well as discrete HII regions) is essential to ...
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