SwePub
Sök i LIBRIS databas

  Utökad sökning

WFRF:(Birkinshaw Mark)
 

Sökning: WFRF:(Birkinshaw Mark) > Evidence of AGN fee...

Evidence of AGN feedback and sloshing in the X-ray luminous NGC 1550 galaxy group

Kolokythas, Konstantinos (författare)
North-West University
O'Sullivan, Ewan (författare)
Harvard-Smithsonian Center for Astrophysics
Giacintucci, Simona (författare)
Naval Research Laboratory
visa fler...
Worrall, Diana M. (författare)
University of Bristol
Birkinshaw, Mark (författare)
University of Bristol
Raychaudhury, Somak (författare)
University of Birmingham,Inter-University Centre for Astronomy and Astrophysics (IUCAA),Presidency University
Horellou, Cathy, 1967 (författare)
Chalmers tekniska högskola,Chalmers University of Technology
Intema, Huib (författare)
Universiteit Leiden (UL),Leiden University (UL)
Loubser, Ilani (författare)
North-West University
visa färre...
 (creator_code:org_t)
2020-06-02
2020
Engelska.
Ingår i: Monthly Notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966. ; 496:2, s. 1471-1487
  • Tidskriftsartikel (refereegranskat)
Abstract Ämnesord
Stäng  
  • We present results from Giant Metrewave Radio Telescope and Chandra observations of the NGC 1550 galaxy group. Although previously thought of as relaxed, we show evidence that gas sloshing and active galactic nucleus (AGN) heating have affected the structure of the system. The 610 and 235 MHz radio images show an asymmetric jet-lobe structure with a total size of similar to 33 kpc, with a sharp kink at the base of the more extended western jet, and bending of the shorter eastern jet as it enters the lobe. The 235-610 MHz spectral index map shows that both radio lobes have steep spectral indices (alpha(610)(235) >= -1.5), indicating the presence of an old electron population. The X-ray images reveal an asymmetric structure in the hot gas correlated with the radio structure, as well as potential cavities coincident with the radio lobes, with rims and arms of gas that may have been uplifted by the cavity expansion. The X-ray residual map reveals an arc-shaped structure to the east that resembles a sloshing cold front. Radio spectral analysis suggests a radiative age of about 33 Myr for the source, comparable to the sloshing time-scale and dynamical estimates of the age of the lobes. An estimate of the mechanical energy required to inflate the cavities suggests that the AGN of NGC 1550 is capable of balancing radiative losses from the intragroup medium (IGM) and preventing excessive cooling, providing that the AGN jets are efficiently coupled to the IGM gas. In conclusion, we find evidence of sloshing motions from both radio and X-ray structures, suggesting that NGC 1550 was perturbed by a minor merger or infalling galaxy about 33 Myr ago.

Ämnesord

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Fysik -- Atom- och molekylfysik och optik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Atom and Molecular Physics and Optics (hsv//eng)
NATURVETENSKAP  -- Biologi -- Strukturbiologi (hsv//swe)
NATURAL SCIENCES  -- Biological Sciences -- Structural Biology (hsv//eng)

Nyckelord

jets
galaxy evolution
AGN
galaxies: groups: general

Publikations- och innehållstyp

art (ämneskategori)
ref (ämneskategori)

Hitta via bibliotek

Till lärosätets databas

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 Stäng

Kopiera och spara länken för att återkomma till aktuell vy