@inproceedings{fce618d96a924ea18a102e92e9f04935,
title = "The physical structure of magellanic cloud HII regions",
abstract = "This paper presents some of the first results of a project aimed at determining in detail the physical conditions of star-forming regions. The project uses spectroscopic data obtained of 17 HII regions in the SMC and LMC. The data set consists of ISO-SWS, ISO-LWS and optical spectroscopic data covering a spectral range from 0.35 mu m to 198 mu m. The combination of optical and infrared data makes it possible to derive the detailed physical structure of an HII region. Quantities derived from this structure, e.g. improved chemical abundances and excitation source, will provide a link to the star-forming properties of these regions.",
keywords = "Magellanic Clouds, interstellar medium, elemental abundances, WAVELENGTH SPECTROMETER",
author = "{van der Hulst}, JM",
year = "1999",
language = "English",
isbn = "92-9092-708-9",
series = "ESA SPECIAL PUBLICATIONS",
publisher = "EUROPEAN SPACE AGENCY",
pages = "985--988",
editor = "P Cox and MF Kessler",
booktitle = "UNIVERSE AS SEEN BY ISO, VOLS I AND II",
note = "Conference on the Universe as Seen by ISO ; Conference date: 20-10-1998 Through 23-10-1998",
}