Preprint
ISM Properties in Low-Metallicity Environments II. The Dust Spectral Energy Distribution of NGC 1569
Abstract
We present new 450 and 850 microns SCUBA data of the dwarf galaxy NGC 1569.
We construct the mid-infrared to millimeter SED of NGC 1569, using ISOCAM,
Authors
Galliano F; Madden SC; Jones AP; Wilson CD; Bernard J-P; Peintre FL
Publication date
June 10, 2003
DOI
10.48550/arxiv.astro-ph/0306192
Preprint server
arXiv