Star Formation and the ISM in Dwarf Galaxies

Simple item page
dc.creatorYoung, L. M.
dc.creatorvan Zee, L.
dc.creatorDohm-Palmer, R. C.
dc.creatorLo, K. Y.
dc.date2000-09-05
dc.date.accessioned2026-07-07T13:02:30Z
dc.date.available2026-07-07T13:02:30Z
dc.descriptionHigh spatial and spectral resolution observations of the atomic interstellar medium in nearby dwarf galaxies reveal evidence for warm and cold neutral gas, just like the phases in our own Galaxy. The cold or quiescent phase (about 20% of the HI in the galaxies studied, except for LGS 3) seems to be associated with star formation activity--- it may mark the regions where the conditions are right for star formation. These results help to explain the patterns of star formation activity which are seen in color-magnitude data for the dwarf irregulars.
dc.description5 pages, 2 figures; to appear in the proceedings of the conference "Gas and Galaxy Evolution" (ASP Conference Series), eds. J. Hibbard, M. Rupen, and J. van Gorkom
dc.identifierhttps://arxiv.org/abs/astro-ph/0009069
dc.identifierhttp://arxiv.org/abs/astro-ph/0009069
dc.identifierASP Conf.Ser.240:187-191,2001
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/226469
dc.subjectAstrophysics
dc.titleStar Formation and the ISM in Dwarf Galaxies
dc.typetext

Files

Collections

arXiv