The Structure of the Local Universe and the Coldness of the Cosmic Flow
| dc.creator | van de Weygaert, Rien | |
| dc.creator | Hoffman, Yehuda | |
| dc.date | 1999-09-06 | |
| dc.date.accessioned | 2026-07-25T21:14:58Z | |
| dc.description | Unlike the substantial coherent bulk motion in which our local patch of the Cosmos is participating, the amplitude of the random motions around this large scale flow seems to be surprisingly low. Attempts to invoke global explanations to account for this coldness of the local cosmic velocity field have not yet been succesfull. Here we propose a different view on this cosmic dilemma, stressing the repercussions of our cosmic neighbourhood embodying a rather uncharacteristic region of the Cosmos. Suspended between two huge mass concentrations, the Great Attractor region and the Perseus-Pisces chain, we find ourselves in a region of relatively low density yet with a very strong tidal shear. By means of constrained realizations of our local Universe, based on Wiener-filtered reconstructions inferred from the Mark III catalogue of galaxy peculiar velocities, we show that indeed this configuration may induce locally cold regions. Hence, the coldness of the local flow may be a cosmic variance effect. | |
| dc.description | Contribution to ``Cosmic Flows. Towards an Understanding of Large-Scale Structure'', Workshop Victoria B.C., July 1999, eds. S. Courteau, M. Strauss, and J. Willick (ASP). 8 pages of LaTeX including 4 postscript figures. Uses psfig | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9909103 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9909103 | |
| dc.identifier.uri | https://dspace.dare.co.zw/handle/123456789/77708 | |
| dc.subject | Astrophysics | |
| dc.title | The Structure of the Local Universe and the Coldness of the Cosmic Flow | |
| dc.type | text |