On the angular momentum history of galactic discs

Abstract

ABSTRACT The stellar mass, size, and rotational velocity of galactic discs all grow from redshift ∼2 to the present by amounts that are estimated from observationally derived scaling relations. The product of these three quantities, the angular momentum of stellar discs, is then estimated to grow by a remarkably large factor, between ∼20 and ∼50, whereas other evidences suggest a more moderate increase. This requires that the specific angular momentum of the accreted gas should systematically increase with time while remaining corotational with the disc over most of the last ∼10 Gyr. Thus, the baryonic gas vorticity of the circumgalactic medium appears to emerge as a major driver in galaxy evolution, and this Letter is meant to attract attention on the sheer size of the angular momentum increase and on the need to explore to which extent this can be observed in nature and/or in simulations.