SwePub
Sök i LIBRIS databas

  Extended search

onr:"swepub:oai:DiVA.org:su-221087"
 

Search: onr:"swepub:oai:DiVA.org:su-221087" > MUSE-ALMA Haloes - ...

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist

MUSE-ALMA Haloes - IX. Morphologies and stellar properties of gas-rich galaxies

Karki, Arjun (author)
Kulkarni, Varsha P. (author)
Weng, Simon (author)
show more...
Péroux, Celine (author)
Augustin, Ramona (author)
Hayes, Matthew J., 1977- (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Ayromlou, Mohammadreza (author)
Kacprzak, Glenn G. (author)
Howk, J. Christopher (author)
Szakacs, Roland (author)
Klitsch, Anne (author)
Hamanowicz, Aleksandra (author)
Fresco, Alejandra (author)
Zwaan, Martin A. (author)
Biggs, Andrew D. (author)
Fox, Andrew J. (author)
Kassin, Susan (author)
Kuntschner, Harald (author)
show less...
 (creator_code:org_t)
2023
2023
English.
In: Monthly notices of the Royal Astronomical Society. - 0035-8711 .- 1365-2966. ; 524:4, s. 5524-5547
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • Understanding how galaxies interact with the circumgalactic medium (CGM) requires determining how galaxies’ morphological and stellar properties correlate with their CGM properties. We report an analysis of 66 well-imaged galaxies detected in Hubble Space Telescope and Very Large Telescope MUSE observations and determined to be within ±500 km s−1 of the redshifts of strong intervening quasar absorbers at 0.2 ≲ z ≲ 1.4 with H I column densities NHI>1018cm−2�HI>1018cm−2⁠. We present the geometrical properties (Sérsic indices, effective radii, axis ratios, and position angles) of these galaxies determined using GALFIT. Using these properties along with star formation rates (SFRs, estimated using the H α or [O II] luminosity) and stellar masses (M* estimated from spectral energy distribution fits), we examine correlations among various stellar and CGM properties. Our main findings are as follows: (1) SFR correlates well with M*, and most absorption-selected galaxies are consistent with the star formation main sequence of the global population. (2) More massive absorber counterparts are more centrally concentrated and are larger in size. (3) Galaxy sizes and normalized impact parameters correlate negatively with NHI, consistent with higher NHI absorption arising in smaller galaxies, and closer to galaxy centres. (4) Absorption and emission metallicities correlate with M* and specific SFR, implying metal-poor absorbers arise in galaxies with low past star formation and faster current gas consumption rates. (5) SFR surface densities of absorption-selected galaxies are higher than predicted by the Kennicutt–Schmidt relation for local galaxies, suggesting a higher star formation efficiency in the absorption-selected galaxies.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

galaxies
evolution - (galaxies: ) quasars
absorption lines - galaxies
stellar content - galaxies
structure

Publication and Content Type

ref (subject category)
art (subject category)

Find in a library

To the university's database

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist

Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.

 
pil uppåt Close

Copy and save the link in order to return to this view