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18 April 2024

» arxiv » astro-ph/9311043

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Is Dark Matter in Spiral Galaxies Cold Gas? I. Observational Constraints and Dynamical Clues About Galaxy Evolution
D. Pfenniger ; F. Combes ; L. Martinet ;
Date:	18 Nov 1993
Journal:	Astron.Astrophys. 285 (1994) 79-83
Abstract:	Based on dynamical constraints about the Hubble sequence evolution, observational data and a number of "conspiracies", we propose that the dark matter around spiral galaxies is in the form of cold gas, essentially in molecular form and rotationally supported. (full A&A paper (in press) available by anonymous ftp at obssd8.unige.ch in /pub/fractal as postscript file: dm_paper_I.ps (170k), or papers I & II + figures as a compressed tar file dm_papers.Z.tar (2.1 Mb)).
Source:	arXiv, astro-ph/9311043
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