Open AccessStar formation and figure rotation in the early‐type galaxy NGC 2974
Author(s) -
Jeong Hyunjin,
Bureau Martin,
Yi Sukyoung K.,
Krajnović Davor,
Davies Roger L.
Publication year - 2007
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1111/j.1365-2966.2007.11535.x
Subject(s) - physics , astrophysics , star formation , astronomy , galaxy , surface brightness , extinction (optical mineralogy) , lenticular galaxy , stellar population , spiral galaxy , radius , optics , computer security , computer science
We present Galaxy Evolution Explorer ( GALEX ) far‐ultraviolet (FUV) and near‐ultraviolet (NUV) imaging of the nearby early‐type galaxy NGC 2974, along with complementary ground‐based optical imaging. In the ultraviolet, the galaxy reveals a central spheroid‐like component and a newly discovered complete outer ring of radius 6.2 kpc, with suggestions of another partial ring at an even larger radius. Blue FUV–NUV and UV‐optical colours are observed in the centre of the galaxy and from the outer ring outwards, suggesting young stellar populations (≲1 Gyr) and recent star formation in both locations. This is supported by a simple stellar population model which assumes two bursts of star formation, allowing us to constrain the age, mass fraction and surface mass density of the young component pixel by pixel. Overall, the mass fraction of the young component appears to be just under 1 per cent (lower limit, uncorrected for dust extinction). The additional presence of a nuclear and an inner ring (radii 1.4 and 2.9 kpc, respectively), as traced by [O iii ] emission, suggests ring formation through resonances. All three rings are consistent with a single pattern speed of 78 ± 6 km s −1 kpc −1 , typical of S0 galaxies and only marginally slower than expected for a fast bar if traced by a small observed surface brightness plateau. This thus suggests that star formation and morphological evolution in NGC 2974 at the present epoch are primarily driven by a rotating asymmetry (probably a large‐scale bar), despite the standard classification of NGC 2974 as an E4 elliptical.