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The Evolution of Galaxies
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The Evolution of Galaxies


New observational windows at ultraviolet, infrared and millimetric wavelengths (provided by ROSAT, IRAM, IUE, IRAS, ISO) have revealed that galaxies contain a wealth of components: very hot gas, atomic hydrogen, molecules, dust, dark matter.
Alaotsikko
I-Observational Clues
Painos
Softcover reprint of the original 1st ed. 2001
ISBN
9789048158218
Kieli
englanti
Paino
310 grammaa
Julkaisupäivä
1.12.2010
Kustantaja
Springer
Sivumäärä
636