Converting H alpha luminosities into star formation rates

That is, local MS stars located at a dis- tance shorter than ∼2.5 kpc are not affected by the presence of the star-forming region G61.48 +0.09, but more distant MS stars have

Even the most metal-deficient galaxies in the local universe formed from matter that was already preenriched by a previous star formation episode, and the determination of the

We aim at identifying the least massive population of the solar metallicity, young (120 Myr), nearby (133.5 pc) Pleiades star cluster with the ultimate goal of understanding

• 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

A comparison between the radio and X-ray populations in Orion shows that the radio detections so far have been strongly biased to the brighter X-ray stars. This supports the

The starburst galaxies from the Lehnert & Heckman (1996) sample have a much lower areal star formation rate. Despite having star-forming regions around 6 times larger on

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