Effect of different stellar galactic environments on planetary discs - I. The solar neighbourhood and the birth cloud of the Sun

Simulate one game until a node (=position) L of T (thanks to bandit algorithms); put this simulation S in memory..

Les podia dorsaux sont longs, coniques, terminés par une petite ventouse soutenue par un disque calcaire très réduit; ces podia sont répartis sur une dizaine

To answer this question, we will derive site-specific power laws relating the horizontal travel distance ∆L 0 to the unstable volume V, using a purely empirical approach, a

Therefore, in order to appropriately model the transport of dust and its associated optical properties and mass impacts, dust models must attempt to capture both the broad size range

Olivier Evrard (1), Guillaume Nord (2), Olivier Cerdan (3), Véronique Souchère (4), Yves Le Bissonnais (5), and Philippe Bonté (1).. (1) Laboratoire des Sciences du Climat et

Mais lorsque je suis entré dans son bureau, je vis encore une fois Médine.. Mais cette fois-ci elle était en présence de tante Adjara, sa tutrice et de

This was concluded from the absence of more rapid growth of RP037 on PHE in co-cultures with a lipopeptide-producing strain (PCL1445) compared to a non-lipopeptide isogenic

We then identify in (2.7) a leading term of size N δt , which corresponds to the statistical error in a Monte-Carlo method for random variables of variance δt, and a remaining