Spatially resolved star formation history along the disk of M82 using multi-band photometric data

• 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

Díaz Soto has raised the point about banning religious garb in the ―public space.‖ He states, ―for example, in most Spanish public Universities, there is a Catholic chapel

Using a combination of optical photometry and spectroscopy we esti- mate stellar masses, ages, and foreground extinction values of the brightest part of the population

The recent work by González Delgado et al., 2016 , using data from the Calar Alto Legacy Integral Field Area Survey (CAL- IFA, see Walcher et al., 2014 ) data, shows that most of

By measuring the two-point correlation function of galaxy populations that differ in redshift, color, luminosity, star-formation history and bias, and using high-resolution

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

In summary, from the cluster analysis of individual bright knots and from the integrated photometry of the whole complex, there are clear indications that there is a complex

In this work we use optical imaging and integral field spec- troscopy (IFS) to study the impact of the minor merger on the star formation properties of the individual galaxies of