星系的紫外形貌
天体物理学
2015-06-24 v1
摘要
真空紫外光提供了对星系形貌、星际演化和星际物质的独特视角，这在解释高红移星系及宇宙星际形成史方面尤为重要。本文综述了自 1990 年来对星系的紫外成像研究。
引用
@article{arxiv.astro-ph/9706265,
title = {The Ultraviolet Morphology of Galaxies},
author = {Robert W. O'Connell},
journal= {arXiv preprint arXiv:astro-ph/9706265},
year = {2015}
}
备注
10 pages; tar.gz file includes LaTeX text file, 6 low-resolution PostScript figures, and 3 style files. For *.ps.gz file with full res figures, see http://www.astro.virginia.edu/~rwo/ Paper to be published in "The Ultraviolet Universe at Low and High Redshift" ed. W. H. Waller (AIP Press) 1997