SwePub
Tyck till om SwePub Sök här!
Sök i LIBRIS databas

  Extended search

WFRF:(Masegosa J.)
 

Search: WFRF:(Masegosa J.) > BERGVALL N > Cumming Robert 1967 > Stellar dynamics of...

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

Stellar dynamics of blue compact galaxies - II. Further indications of a merger in ESO 338-IG04

Cumming, Robert, 1967 (author)
Stockholms universitet,Institutionen för astronomi
Fathi, Kambiz (author)
Stockholms universitet,Institutionen för astronomi
Östlin, Göran (author)
Stockholms universitet,Institutionen för astronomi
show more...
Marquart, Thomas (author)
Uppsala universitet,Institutionen för astronomi och rymdfysik,Uppsala University
Marquez, I. (author)
Instituto de Astrofisica de Andalucía (IAA),Institute of Astrophysics of Andalusia (IAA)
Masegosa, J. (author)
Instituto de Astrofisica de Andalucía (IAA),Institute of Astrophysics of Andalusia (IAA)
Bergvall, N. (author)
Uppsala universitet,Institutionen för astronomi och rymdfysik,Uppsala University
Amram, P. (author)
Centre national de la recherche scientifique (CNRS)
show less...
 (creator_code:org_t)
2008-01-02
2008
English.
In: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 479:3, s. 725-733
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • Context. Luminous blue compact galaxies, common at z similar to 1 but now relatively rare, show disturbed kinematics in emission lines. Aims. As part of a programme to understand their formation and evolution, we have investigated the stellar dynamics of a number of nearby objects in this class. Methods. We obtained long-slit spectra with VLT/FORS2 in the spectral region covering the near-infrared calcium triplet. In this paper we focus on the well-known luminous blue compact galaxy ESO338-IG04 (Tololo 1924 - 416). A previous investigation, using Fabry-Perot interferometry, showed that this galaxy has a chaotic Ha velocity field, indicating that either the galaxy is not in dynamical equilibrium or that Ha does not trace the gravitational potential due to feedback from star formation. Results. Along the apparent major axis, the stellar and ionised gas velocities for the most part follow each other. The chaotic velocity field must therefore be a sign that the young stellar population in ESO338-IG04 is not in dynamical equilibrium. The most likely explanation, which is also supported by its morphology, is that the galaxy has experienced a merger and that this has triggered the current starburst. Summarising the results of our programme so far, we note that emission-line velocity fields are not always reliable tracers of stellar motions, and go on to assess the implications for kinematic studies of similar galaxies at intermediate redshift.

Subject headings

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

Keyword

galaxies : evolution
galaxies : kinematics and dynamics
galaxies : individual : ESO338-IG04
galaxies : starburst
galaxies : interactions
Physics
Fysik
Extragalactical astronomy

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