What is the behavior of the ISM in the SMC?
arXiv:astro-ph/0008327 · doi:10.1023/A:1012787829247
Abstract
We describe quantitatively the neutral hydrogen (HI) and dust content of the interstellar medium (ISM) in the Small Magellanic Cloud (SMC), using the spatial power spectrum. The velocity modification of the HI density power spectrum is investigated and discussed.
4 pages, 2 figures, to appear in the proceedings of "The Evolution of Galaxies: I Observational Clues", eds. J.M. Vilchez, G. Stasinska & E. Perez