The physical structure of Magellanic Cloud HIIregions*

Autor: Vermeij, R., Damour, F., van der Hulst, J. M., Baluteau, J-.P., Vermeij, R., Damour, F., van der Hulst, J. M., Baluteau, J-.P.
Zdroj: Astronomy and Astrophysics; August 2002, Vol. 390 Issue: 2 p649-665, 17p
Abstrakt: We present infrared and optical spectroscopic data for 11 HIIregions and one Supernova Remnant in the Large and Small Magellanic Cloud. The infrared data have been obtained with the Short Wavelength Spectrometer and Long Wavelength Spectrometer on board the Infrared Space Observatoryas part of a Guaranteed Time Program on HIIregions in Local Group Galaxies. Aim of this project is to give a new and improved analysis of the physical structure of the sample HIIregions by combining as much spectral data as possible. A detailed account is given here of the reduction process, and the quality and reliability of the presented fluxes are discussed.
Databáze: Supplemental Index