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

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A90259%2F23%3A00583591" target="_blank" >RIV/67985815:90259/23:00583591 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1017/pasa.2023.14" target="_blank" >https://doi.org/10.1017/pasa.2023.14</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1017/pasa.2023.14" target="_blank" >10.1017/pasa.2023.14</a>

Result language
angličtina
Original language name
VERTICO V: The environmentally driven evolution of the inner cold gas discs of Virgo cluster galaxies
Original language description
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 (S-*), H I (S-H I), and molecular gas (S-mol) 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 S-H I of the remaining gas even in the central 1.2 kpc.
Czech name
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Czech description
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Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)

Publication year
2023
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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