Toward Unbiased Abundance Measurements in Inhomogeneous $\mathrm{H\,II}$ Regions
ArXiv 2607.05295 (2026)
Exploring the synergies of $[\mathrm{O\,II}]λ3727$ with MUSE spectroscopy in PHANGS H II regions
ArXiv 2607.00408 (2026)
Revisiting Ram Pressure Stripping in Wolf–Lundmark–Melotte: No Evidence for Stripped HIwith Local Group L-Band Survey
Astronomical Journal 172:1 (2026)
Abstract:
We analyze H i 21 cm observations of the Local Group dwarf galaxy Wolf–Lundmark–Melotte (WLM) from the Local Group L-Band Survey to search for evidence of ram pressure stripping. While previous MeerKAT-16 observations of WLM showed evidence for off-galaxy atomic gas emission with a geometry suggestive of ram pressure stripping, our observations find no evidence for this stripped gas. We demonstrate that our observations would be sensitive to the claimed detections and suggest that an uncorrected observational flaw with the MeerKAT data led to the apparent off-galaxy emission. The lack of off-galaxy emission obviates the need for uncharacteristically high values of the density of the intergalactic medium in this region.Erratum: “Cloud-scale Gas Properties, Depletion Times, and Star Formation Efficiency per Freefall Time in PHANGS–ALMA” (2025, ApJ, 985, 14)
The Astrophysical Journal American Astronomical Society 1003:2 (2026) 248
From gas to stars along the spiral wave: CO, HCN, and star formation variations across the spiral arms in NGC 4321 and M51
ArXiv 2605.05302 (2026)