
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.
- Undertitel
- I-Observational Clues
- Redaktör
- José M. Vilchez, Grazyna Stasinska, Enrique Pérez
- Upplaga
- Reprinted from ASTROPHYSICS AND SPACE SCIENCE, 277, 2001
- ISBN
- 9781402000010
- Språk
- Engelska
- Vikt
- 446 gram
- Utgivningsdatum
- 2001-12-31
- Sidor
- 636