Observations of hydroxyl in early-type galaxies

Abstract

We used Arecibo Observatory and the Green Bank Telescope to observe OH in twelve early-type galaxies with known reservoirs of dense gas. We present three new detections of OH in absorption in the 1667 MHz line. One objective of our survey was to find evidence of molecular outflows, but our sensitivity, and the strength of the OH absorption, were insufficient to detect outflows. The detected sources have infrared luminosities and dust temperatures among the lowest of any galaxy detected in OH absorption. The ratio $L_{\mathrm{HCN}}/L_{\mathrm{CO}}$, a measure of the dense gas fraction in galaxies, is a powerful selector of OH megamasers for galaxies with high infrared luminosity. In early-type galaxies, which have much lower infrared luminosities, $L_{\mathrm{HCN}}/L_{\mathrm{CO}}$ is also a promising tool for discovering OH, but in absorption rather than in maser emission. In addition to dense molecular gas, a radio continuum source and a favorable line-of-sight to the observer are likely key factors in detecting OH absorbers.

arXiv comment8 pages, accepted to MNRAS

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Cited by in corpus (3)

• Evidence of boosted 13CO/12CO ratio in early-type galaxies in dense environments
• Blind HI and OH absorption line search: first results with MALS and uGMRT processed using ARTIP
• OH in the diffuse interstellar medium: physical modelling and prospects with upcoming SKA precursor/pathfinder surveys