2003/01/13 by J. S. Gallagher, G. J. Madsen, R. J. Reynolds +3 · 1 citation
Physics and Astronomy · #Astrophysics and Star Formation Studies #Galaxies: Formation, Evolution, Phenomena #Gamma-ray bursts and supernovae #astro-ph
paper · pdf · doi:10.1086/373951
published as Astrophys.J. 588 (2003) 326-330 · 10 pages, 2 figures, AASTeX two-column format. Accepted for publication in The Astrophysical Journal
arxiv created 2003/01/13 · openalex publication_date 2003/05/01 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/01
The Wisconsin Hα Mapper has been used to set the first deep upper limits on the intensity of diffuse Hα emission from warm ionized gas in the Draco and Ursa Minor dwarf spheroidal galaxies (dSphs). Assuming a velocity dispersion of 15 km s -1 for the ionized gas, we set limits of I Hα ≤ 0.024 R and I Hα ≤ 0.021 R for the Draco and Ursa Minor dSphs, respectively, averaged over our 1° circular beam. Adopting a simple model for the ionized interstellar medium, these limits translate to upper bounds on the mass of ionized gas of ≲10% of the stellar mass, or ~10 times the upper limits for the mass of neutral hydrogen. Note that the Draco and Ursa Minor dSphs could contain substantial amounts of interstellar gas, equivalent to all of the gas injected by dying stars since the end of their main star-forming episodes ≳8 Gyr in the past, without violating these limits on the mass of ionized gas.