The Millennium Arecibo 21-cm Absorption Line Survey: Extolling the Analysis Procedures

Simple item page
dc.creatorHeiles, Carl
dc.date2002-02-14
dc.date.accessioned2026-07-07T02:02:48Z
dc.date.available2026-07-07T02:02:48Z
dc.descriptionWe have recently completed the analysis of a survey of the HI line in emission/absorption against 79 radio sources. Our CNM temperatures are about half those of previous authors and we find a substantial quantity of thermally unstable WNM. These results are somewhat controversial. Here we discuss the analysis procedures to illustrate explicitly why the results are reliable.
dc.description4 pages, 1 figure. Presented at "Seeing Through the Dust - The Detection of HI and the Exploration of the ISM Galaxies"
dc.identifierhttps://arxiv.org/abs/astro-ph/0202266
dc.identifierhttp://arxiv.org/abs/astro-ph/0202266
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4171
dc.subjectAstrophysics
dc.titleThe Millennium Arecibo 21-cm Absorption Line Survey: Extolling the Analysis Procedures
dc.typetext

Files

Collections

arXiv