Forskning ved Københavns Universitet - Københavns Universitet

Forside

MUSE Analysis of Gas around Galaxies (MAGG) - I: Survey design and the environment of a near pristine gas cloud at z approximate to 3.5

Publikation: Bidrag til tidsskriftTidsskriftartikelForskningfagfællebedømt

Dokumenter

  • stz3066

    Forlagets udgivne version, 3,2 MB, PDF-dokument

  • Emma K. Lofthouse
  • Michele Fumagalli
  • Matteo Fossati
  • John M. O'Meara
  • Michael T. Murphy
  • Christensen, Lise Bech
  • J. Xavier Prochaska
  • Sebastiano Cantalupo
  • Richard M. Bielby
  • Ryan J. Cooke
  • Elisabeta Lusso
  • Simon L. Morris

We present the design, methods, and first results of the MUSE Analysis of Gas around Galaxies (MAGG) survey, a large programme on the Multi-Unit Spectroscopic Explorer (MUSE) instrument at the Very Large Telescope (VLT), which targets 28 z > 3.2 quasars to investigate the connection between optically thick gas and galaxies at z similar to 3-4. MAGG maps the environment of 52 strong absorption line systems at z greater than or similar to 3, providing the first statistical sample of galaxies associated with gas-rich structures in the early Universe. In this paper, we study the galaxy population around a very metal poor gas cloud at z approximate to 3.53 towards the quasar J124957.23-015928.8. We detect three Ly alpha emitters within less than or similar to 200 km s(-1) of the cloud redshift, at projected separations less than or similar to 185 kpc (physical). The presence of star-forming galaxies near a very metal-poor cloud indicates that metal enrichment is still spatially inhomogeneous at this redshift. Based on its very low metallicity and the presence of nearby galaxies, we propose that the most likely scenario for this Lyman Limit System (LLS) is that it lies within a filament which may be accreting on to a nearby galaxy. Taken together with the small number of other LLSs studied with MUSE, the observations to date show a range of different environments near strong absorption systems. The full MAGG survey will significantly expand this sample and enable a statistical analysis of the link between gas and galaxies to pin down the origin of these diverse environments at z approximate to 3-4.

OriginalsprogEngelsk
TidsskriftMonthly Notices of the Royal Astronomical Society
Vol/bind491
Udgave nummer2
Sider (fra-til)2057-2074
Antal sider18
ISSN0035-8711
DOI
StatusUdgivet - 2 jan. 2020

Links

Antal downloads er baseret på statistik fra Google Scholar og www.ku.dk


Ingen data tilgængelig

ID: 248237870