Helium Ionization in the Diffuse Ionized Gas Surrounding UCH ii Regions

• Published in: The Astrophysical journal Vol. 838; no. 2; pp. 144 - 160
• Main Authors: Roshi, D. Anish, Churchwell, E., Anderson, L. D.
• Format: Journal Article
• Language: English
• Published: Philadelphia The American Astronomical Society 01-04-2017; IOP Publishing
• Subjects: ABSORPTION; Astrophysics; ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; Continuum radiation; COSMIC DUST; COSMIC GASES; Deposition; DETECTION; Dust; EMISSION; GALAXIES; Galaxy: general; H II regions; HELIUM; Helium ions; HYDROGEN; IONIZATION; Ionizing radiation; IONIZING RADIATIONS; ISM: general; ISM: lines and bands; ISM: structure; Low mass stars; MASS; Massive stars; PHOTONS; Radiation; radio lines: ISM; RECOMBINATION; regions; STARS
• ISSN: 0004-637X; 1538-4357
• DOI: 10.3847/1538-4357/aa662b

We present measurements of the singly ionized helium-to-hydrogen ratio ( ) toward diffuse gas surrounding three ultracompact H ii (UCH ii) regions: G10.15-0.34, G23.46-0.20, and G29.96-0.02. We observe radio recombination lines of hydrogen and helium near 5 GHz using the GBT to measure the ratio. The measurements are motivated by the low helium ionization observed in the warm ionized medium and in the inner Galaxy diffuse ionized regions. Our data indicate that the helium is not uniformly ionized in the three observed sources. Helium lines are not detected toward a few observed positions in sources G10.15-0.34 and G23.46-0.20, and the upper limits of the ratio obtained are 0.03 and 0.05, respectively. The selected sources harbor stars of type O6 or hotter as indicated by helium line detection toward the bright radio continuum emission from the sources with mean value 0.06 0.02. Our data thus show that helium in diffuse gas located a few parsecs away from the young massive stars embedded in the observed regions is not fully ionized. We investigate the origin of the nonuniform helium ionization and rule out the possibilities (a) that the helium is doubly ionized in the observed regions and (b) that the low values are due to additional hydrogen ionizing radiation produced by accreting low-mass stars. We find that selective absorption of ionizing photons by dust can result in low helium ionization but needs further investigation to develop a self-consistent model for dust in H ii regions.