• Aucun résultat trouvé

A statistical and multi-wavelength study of star formation in galaxies

N/A
N/A
Protected

Academic year: 2021

Partager "A statistical and multi-wavelength study of star formation in galaxies"

Copied!
266
0
0

Texte intégral

Loading

Figure

Figure 1.1 – Estimated star formation history (SFH) of the Milky Way (MW). On the y axis is the MW’s star formation rate (SFR), in units of solar masses per year (M ⊙ /yr), and on the x axis is the lookback time in bilion years, i.e., today is on the left,
Figure 1.4 – Correlation between the surface density of star formation rate (Σ SFR ) and the surface density of hydrogen gas (Σ gas ), the  so-called Schmidt–Kennicutt law, adapted from Daddi et al
Figure 3.3 – Evolution of the star- star-forming galaxy stellar mass  func-tion with redshift in the three  CAN-DELS fields GOODS–South, UDS, and COSMOS for galaxies brighter than H = 26
Figure 3.6 – Stacked SEDs of our star-forming mass-selected samples in bins of redshift (horizontally) and stellar mass (vertically)
+7

Références

Documents relatifs

tion from NYC Dept.. Use Groups Compared. Land area where New York City's use groups are allowed to locate as-of-right in Manhattan. Note that these figures do not

(Fig. Même silhouette mais plastes différents, cependant tous deux sont conformes aux défini- tions données par Cox. Toutefois, nous avons ren- contré dans les 2

As one assessment to cover the partial failing of GPR technique in detecting the low and non-metallic landmines buried in the conductive environment, simple forward modeling of

The liquid slosh within each carbon dioxide tank changes the A matrix of the system with respect to time giving the SPHERES satellite the time-varying

bonates on Mars: A) Near-infrared spectra of terrestrial car- bonate minerals in grey [9] and carbonate rocks from terrestrial impact craters in colors, B) CRISM spectra from

The solutions are used to study the effect of initial average concentration, variance, correlation length, cross correlation, and the size of the domain on the A þ B * C

En effet, entre chaque deux plaques de PVC superposées, et en fonction du nombre de couches de renfort, soit une couche de renfort textile est positionnée, soit une ficelle à

observed number of events predicted for the MiniBooNE sample and the size of the reduced systematic uncertainties after applying the SciBooNE corrections are shown in Table III.. As