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Search: WFRF:(McHardy I.) > Chalmers University of Technology > LeMMINGs: V. Nuclea...

LeMMINGs: V. Nuclear activity and bulge properties: A detailed multi-component decomposition of e -MERLIN Palomar galaxies with HST

Dullo, B. T. (author)
Knapen, J. H. (author)
Universidad de la Laguna,University of La Laguna,Instituto de Astrofísica de Canarias
Beswick, R. J. (author)
University of Manchester
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Baldi, R. D. (author)
University of Southampton,Istituto di Radioastronomia
Williams, D. R.A. (author)
University of Manchester
McHardy, I. M. (author)
University of Southampton
Gallagher III, J. S. (author)
University of Wisconsin Madison
Aalto, Susanne, 1964 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Argo, M. K. (author)
University of Central Lancashire
Gil De Paz, A. (author)
Klockner, H. R. (author)
Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
Marcaide, J.M. (author)
Mundell, C. G. (author)
University of Bath
Mutie, I. (author)
Technical University of Kenya,University of Manchester
Saikia, P. (author)
New York University Abu Dhabi
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 (creator_code:org_t)
2023
2023
English.
In: Astronomy and Astrophysics. - 0004-6361 .- 1432-0746. ; 675
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • We used high-resolution HST imaging and e-MERLIN 1.5-GHz observations of galaxy cores from the LeMMINGs survey to investigate the relation between optical structural properties and nuclear radio emission for a large sample of galaxies. We performed accurate, multi-component decompositions of new surface brightness profiles extracted from HST images for 163 LeMMINGs galaxies and fitted up to six galaxy components (e.g. bulges, discs, AGN, bars, rings, spiral arms, and nuclear star clusters) simultaneously with Sérsic and/or core-Sérsic models. By adding such decomposition data for ten LeMMINGs galaxies from our past work, the final sample of 173 nearby galaxies (102 Ss, 42 S0s, 23 Es, plus six Irr) with a typical bulge stellar mass of M∗,bulge ~ 106 -1012.5 M⊙ encompasses all optical spectral classes: low-ionisation nuclear emission-line region (LINER), Seyfert, Absorption Line Galaxy (ALG), and H′ ¯II. We show that the bulge mass can be significantly overestimated in many galaxies when components such as bars, rings, and spirals are not included in the fits. We additionally implemented a Monte Carlo method to determine errors on the bulge, disc, and other fitted structural parameters. Moving (in the opposite direction) across the Hubble sequence, that is from the irregular to elliptical galaxies, we confirm that bulges become larger, more prominent, and round. Such bulge dominance is associated with a brighter radio core luminosity. We also find that the radio detection fraction increases with bulge mass. At M∗,bulge ≫ 1011 M⊙, the radio detection fraction is 77%, declining to 24% for M∗,bulge < 1010 M⊙. Furthermore, we observe that core-Sérsic bulges tend to be systematically round and to possess high radio core luminosities and boxy-distorted or pure elliptical isophotes. However, there is no evidence for the previously alleged strong tendency of galaxies'central structures (i.e. a sharp Sérsic, core-Sérsic dichotomy) with their radio loudness, isophote shape, and flattening.

Subject headings

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

Keyword

Galaxies: elliptical and lenticular
CD
Galaxies: photometry
Galaxies: nuclei
Galaxies: spiral
Radio continuum: galaxies
Galaxies: structure

Publication and Content Type

art (subject category)
ref (subject category)

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