• Aucun résultat trouvé

Échange de Billets de Banque Canadiens de 100 $ (A)

N/A
N/A
Protected

Academic year: 2021

Partager "Échange de Billets de Banque Canadiens de 100 $ (A)"

Copied!
2
0
0

Texte intégral

(1)

´

Echange de Billets de Banque – Canada (A)

Calculez combien d’argent est rendu pour chaque transaction.

Coˆut des Articles Montant Pay´e Argent Rendu

1. 70,25 $ 100,00 $ 2. 65,02 $ 100,00 $ 3. 90,85 $ 100,00 $ 4. 60,23 $ 100,00 $ 5. 29,63 $ 100,00 $

Images de billets de banque utilis´ees avec la permission de la Banque du Canada.

(2)

´

Echange de Billets de Banque – Canada (A) R´eponses

Calculez combien d’argent est rendu pour chaque transaction.

Coˆut des Articles Montant Pay´e Argent Rendu

1. 70,25 $ 100,00 $ 29,75 $ 2. 65,02 $ 100,00 $ 34,98 $ 3. 90,85 $ 100,00 $ 9,15 $ 4. 60,23 $ 100,00 $ 39,77 $ 5. 29,63 $ 100,00 $ 70,37 $

Images de billets de banque utilis´ees avec la permission de la Banque du Canada.

Références

Documents relatifs

Comparing assembly statistics and differential gene expression analysis results obtained from methodology 2 and methodology 3, further downstream functional analyses were

This pro- duction of carbon-rich DOM may lead to the formation of a large pool of DOM that is not stoichiometrically locked into the Redfield C : N ratio and accumulates in the

Dans les phrases suivantes, soulignez la phrase subordonnée et dites si le subordonnant est simple ou complexe.. a) Quand ils eurent fini de manger, ils rentrèrent dans le salon,

These data show that oce- anic crust generated at slow- and ultra- slow mid-ocean ridge spreading centers can consist of a gabbro massif centered beneath a magmatic ridge segment

The rate constants of the reactions of 1-pentanol, 2-pentanol and 3- pentanol with OH radicals and Cl atoms at T= (298±2) K and P = 760 Torr obtained using the relative rate

To understand the sources contributing to the CIB and to interpret the deep source counts, we have developed a phe- nomenological model that constrains in a simple way the IR

d log(S 24 ) (solid symbols), as a function of the 24 µm flux, in all three MIPS GTO Fields. A completeness correction has been applied. The highest flux bin goes up to 1 Jy.

In x 5 we study the evolution of IR luminosities and stellar masses with redshift and put constraints on the SFRs and timescales for star formation activity in different mass