3 edition of Galactic nebulae and interstellar matter found in the catalog.
Galactic nebulae and interstellar matter
Written in English
Originally published as Neḃuleuses galactiques et matie`re interstellaire. Michel,1954.
|Statement||translated from the French by A.J. Pomerans.|
|The Physical Object|
|Number of Pages||352|
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Galactic nebulae and interstellar matter. London: Hutchinson's Scientific and Technical Publications, (OCoLC) Document Type: Book: All Authors / Contributors: Jean Dufay; Arnold Pomerans.
Additional Physical Format: Online version: Dufay, Jean, Galactic nebulae and interstellar matter. New York, Philosophical Library .
Classes of nebulae. All nebulae observed in the Milky Way Galaxy are forms of interstellar matter—namely, the gas between the stars that is almost always accompanied by solid grains of cosmic dust. Their appearance differs widely, depending not only on the temperature and density of the material observed but also on how the material is spatially situated with respect to the.
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A nebula (Latin for 'cloud' or 'fog'; pl. nebulae, nebulæ or nebulas) is an interstellar cloud of dust, hydrogen, helium and other ionized ally, the term was used to describe any diffused astronomical object, including galaxies beyond the Milky Andromeda Galaxy, for instance, was once referred to as the Andromeda Nebula (and spiral galaxies in general as .