An excessively massive thick disc of the enormous edge-on lenticular galaxy NGC7572статья
Статья опубликована в высокорейтинговом журнале
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Дата последнего поиска статьи во внешних источниках: 19 августа 2020 г.
Аннотация:Galactic discs are known to have a complex multi-layer structure. An in-depth study of the stellar population properties of the thin and thick components can elucidate the formation and evolution of disc galaxies. Even though thick discs are ubiquitous, their origin is still debated.
Here we probe the thick disc formation scenarios by investigating N7572, an enormous edge-on galaxy having R_{25} = 25 kpc and V_{rot} = 370 km/s, which substantially exceeds the Milky Way size and mass. We analysed DECaLS archival imaging and found that the disc of N7572 contains two flaring stellar discs (a thin and a thick disc) with similar radial scales. We collected deep long-slit spectroscopic data using the 6-m Russian BTA telescope and analysed them with a novel technique. We first reconstructed a non-parametric stellar line-of-sight velocity distribution along the radius of the galaxy and then fitted it with two kinematic components accounting for the orbital distribution of stars in thin and thick discs. The old thick disc turned out to be 2.7 times as massive as the intermediate-age thin component, 1.6 x 10^{11} Msun vs. 5.9 x 10^{10} Ms, which is very unusual.
The different duration of the formation epochs evidenced by the [Mg/Fe] values of +0.3 dex and +0.15 dex for the thick and thin discs respectively, their kinematics and the mass ratio suggest that in N7572 we observe a rapidly formed very massive thick disc and an under-developed thin disc, whose growth ended prematurely due to the exhaustion of the cold gas likely because of environmental effects.