Interstellar matter is an important component of our Galaxy although its mass may be less than 10% of the whole system. The structure of the Galaxy is strongly affected by the distribution of interstellar matter and its evolution is mainly determined by the amount of interstellar gas and dust which is available for star formation.
KeywordsDiffuse Light Interstellar Dust Interstellar Extinction Extinction Curve Galactic Latitude
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- Ackermann, G.: 1969, Thesis Heidelberg.Google Scholar
- Johnson, H. L.: 1968, in Nebulae and Interstellar Matter (ed. by. B. M. Middlehurst and L. H. Aller), Univ. of Chicago Press, Chicago, p. 167.Google Scholar
- Klare, G. and Neckel, Th.: 1970, in The Spiral Structure of Our Galaxy, 1AU Symposium No. 38 (ed. by W. Becker and G. Contopoulos), D. Reidel, Dordrecht-Holland, p. 449.Google Scholar
- Mattila, K.: 1970, Thesis Heidelberg.Google Scholar
- Neckel, Th.: 1967, Veröffentl. Landessternw. Heidelberg-Königstuhl 19. Google Scholar