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Table · dataset · 2026

CO-dark gas in compact emission-line galaxies

Listed in IVOA Registry (Virtual Observatory)

Green Pea and Blueberry galaxies are compact, low-metallicity starbursts that provide nearby analogs of high-redshift star-forming systems.

Description

We investigate whether their weak CO emission reflects genuinely small molecular reservoirs or CO-dark gas where independent tracers are available. We compiled 60 strong [OIII]{lambda}5007 compact emission-line galaxies with partially overlapping gas-tracer coverage: ^12^CO(1-0) observations from the Delingha 13.7m telescope, HI 21cm data from Arecibo, GBT, and FAST (ten detections and 41 upper limits), and Herschel/PACS [CII] {lambda}158um data (five detections and four upper limits after excluding merger systems).

Quantitative conclusions are drawn only from detected or physically constraining subsets. Molecular masses were estimated using a metallicity-dependent CO-to-H_2_ conversion factor and the [CII]-to-H_2_ calibration for low-metallicity dwarf galaxies. Two CO upper limits are deep enough to constrain the expected molecular reservoir.

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We also removed major mergers and examined the large-scale environment using the SDSS DR7 VoidFinder catalog. For the five [CII]-detected sources, we find M_H2_^[CII]^~10^9^.0-10^9.7^M_{sun}_ and a median molecular gas depletion time of {tau}_dep,H2_~0.16Gyr, shorter than the ~1Gyr typical of main-sequence galaxies. HI-detected sources have a median atomic depletion time of {tau}_dep,H_~2.6Gyr.

The detected subsets show high gas fractions and short depletion times consistent with rapid gas cycling, but the [CII] result remains limited by small-number statistics. About 39% of the volume-matched sample lies in cosmic voids. CO alone misses a substantial fraction of the star-forming fuel in these low-metallicity starbursts.

Combined HI, [CII], and deep CO constraints are needed to characterize their interstellar medium and CO-dark molecular component.

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