A massive, distant proto cluster at z = 2 47 caught in a phase of rapid formation?

We compare the SFRs, morphologies and gas fractions of six galaxies of MW-like stellar masses to eight from unconstrained simulations and find systematically higher SFRs in the

✴ WEAVE , IFU mode (fov = 2 sq. arcmin, with 1-2.5 arcsec/sparxel) to trace the stellar population of galaxies beyond 3 HLR in a large sample of galaxies covering all

The separation into in-situ and accreted stars indicates that the negative slope partly origi- nates from the in-situ stars, but the steepening of the gradi- ents in the outer

The circularized stellar mass density profiles for the galaxies in our sample, comparing them with similar mass SDSS ETGs and the massive compact galaxies in Szomoru et al..

Topic 2 : The mass distribution in disc galaxies (Bershady’s talk yesterday) S tellar kinematics in gas-dominated Lower Surface Brightness galaxies.. G alaxies at higher

• Stellar kinematic signatures of intermediate mass black holes in nuclear stellar clusters (with T.. Compare star formation history deduced from fit to absorption line spectra

Figure 5 shows that the underlying stellar populations of the local H ii galaxies are compatible with the evolution of LCBGs in the sense that their B
R colors were the same at

The values measured for the radio galaxies can be corrected for their intrinsic velocity dispersions; we have chosen instead to recalibrate the index using template stars of