VERTICO V: The environmentally driven evolution of the inner cold gas discs of Virgo cluster galaxies

Watts, Adam B., Cortese, Luca, Catinella, Barbara, Brown, Toby, Wilson, Christine D., Zabel, Nikki, Roberts, Ian D., Davis, Timothy A. ORCID: https://orcid.org/0000-0003-4932-9379, Thorp, Mallory, Chung, Aeree, Stevens, Adam R.H., Ellison, Sara L., Spekkens, Kristine, Parker, Laura C., Bahé, Yannick M., Villanueva, Vicente, Jiménez-Donaire, María, Bisaria, Dhruv, Boselli, Alessandro, Bolatto, Alberto D. and Lee, Bumhyun 2023. VERTICO V: The environmentally driven evolution of the inner cold gas discs of Virgo cluster galaxies. Publications of the Astronomical Society of Australia 40 , e17. 10.1017/pasa.2023.14

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Abstract

The quenching of cluster satellite galaxies is inextricably linked to the suppression of their cold interstellar medium (ISM) by environmental mechanisms. While the removal of neutral atomic hydrogen (H I) at large radii is well studied, how the environment impacts the remaining gas in the centres of galaxies, which are dominated by molecular gas, is less clear. Using new observations from the Virgo Environment traced in CO survey (VERTICO) and archival H I data, we study the H I and molecular gas within the optical discs of Virgo cluster galaxies on 1.2-kpc scales with spatially resolved scaling relations between stellar ( Σ⋆ ), H I ( ΣHI ), and molecular gas ( Σmol ) surface densities. Adopting H I deficiency as a measure of environmental impact, we find evidence that, in addition to removing the H I at large radii, the cluster processes also lower the average ΣHI of the remaining gas even in the central 1.2 kpc. The impact on molecular gas is comparatively weaker than on the H I, and we show that the lower Σmol gas is removed first. In the most H I-deficient galaxies, however, we find evidence that environmental processes reduce the typical Σmol of the remaining gas by nearly a factor of 3. We find no evidence for environment-driven elevation of ΣHI or Σmol in H I-deficient galaxies. Using the ratio of Σmol -to- ΣHI in individual regions, we show that changes in the ISM physical conditions, estimated using the total gas surface density and midplane hydrostatic pressure, cannot explain the observed reduction in molecular gas content. Instead, we suggest that direct stripping of the molecular gas is required to explain our results.

Item Type:	Article
Date Type:	Published Online
Status:	Published
Schools:	Physics and Astronomy
Publisher:	Cambridge University Press
ISSN:	1323-3580
Date of First Compliant Deposit:	14 September 2023
Date of Acceptance:	9 March 2023
Last Modified:	16 Sep 2023 22:39
URI:	https://orca.cardiff.ac.uk/id/eprint/162519

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