Feeding compact bulges and supermassive black holes with low angular-momentum cosmic gas at high redshift

Details Feeding compact bulges and supermassive black holes with low angular-momentum cosmic gas at high redshift Feeding compact bulges and supermassive black holes with low angular-momentum cosmic gas at high redshift

2011-12-12

arxiv.org/abs/1112.2479v2

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

17 pages, 13 figures, MNRAS accepted

Scientific paper

We use cosmological hydrodynamical simulations to show that a significant fraction of the gas in high redshift rare massive halos falls nearly radially to their very centre on extremely short timescales. This process results in the formation of very compact bulges with specific angular momentum a factor 5-30$smaller than the average angular momentum of the baryons in the whole halo. Such low angular momentum originates both from segregation and effective cancellation when the gas flows to the centre of the halo along well defined cold filamentary streams. These filaments penetrate deep inside the halo and connect to the bulge from multiple rapidly changing directions. Structures falling in along the filaments (satellite galaxies) or formed by gravitational instabilities triggered by the inflow (star clusters) further reduce the angular momentum of the gas in the bulge. Finally, the fraction of gas radially falling to the centre appears to increase with the mass of the halo; we argue that this is most likely due to an enhanced cancellation of angular momentum in rarer halos which are fed by more isotropically distributed cold streams. Such an increasingly efficient funnelling of low-angular momentum gas to the centre of very massive halos at high redshift may account for the rapid pace at which the most massive supermassive black holes grow to reach observed masses around $10^9$M$_\odot$ at an epoch when the Universe is barely 1 Gyr old.

Affiliated with

Also associated with

No associations

Rating

Feeding compact bulges and supermassive black holes with low angular-momentum cosmic gas at high redshift does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Feeding compact bulges and supermassive black holes with low angular-momentum cosmic gas at high redshift, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Feeding compact bulges and supermassive black holes with low angular-momentum cosmic gas at high redshift will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-708656