ALMACAL - III. A combined ALMA and MUSE survey for neutral, molecular, and ionized gas in an H I-absorption-selected system

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F18%3A00540230" target="_blank" >RIV/67985815:_____/18:00540230 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1093/mnras/stx3184" target="_blank" >https://doi.org/10.1093/mnras/stx3184</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1093/mnras/stx3184" target="_blank" >10.1093/mnras/stx3184</a>

Result language
angličtina
Original language name
ALMACAL - III. A combined ALMA and MUSE survey for neutral, molecular, and ionized gas in an H I-absorption-selected system
Original language description
We present a detailed case study of the environment around an intervening Ly alpha absorption line system at z(abs) = 0.633, seen towards the quasar J0423-0130 (z(QSO) = 0.915). We detect with ALMA the (CO)-C-12(2-1), (CO)-C-12(3-2), and 1.2 mm continuum emission from a galaxy at the redshift of the Ly alpha absorber at a projected distance of 135 kpc. From the ALMA detections, we infer interstellar medium conditions similar to those in low-redshift luminous infrared galaxies.
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
2018
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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