A spectral and photometric study of 102 star forming regions in seven spiral galaxies

TL;DR

This study combines spectroscopic and photometric data to analyze 102 star-forming regions across seven spiral galaxies, revealing properties like ages, masses, and extinctions of young massive cluster complexes, and their relation to Milky Way clusters.

Contribution

It provides a comprehensive dataset and analysis of young massive star cluster complexes in multiple galaxies, highlighting their properties and evolutionary sequences.

Findings

Cluster ages are up to 10 Myr.

Masses range from 10^4 to 10^7 solar masses.

Extinction varies between 0 and 3 magnitudes.

Abstract

We present a study of complexes of young massive star clusters (YMCs), embedded in extragalactic giant HII regions, based on the coupling of spectroscopic with photometric and spectrophotometric observations of about 100 star forming regions in seven spiral galaxies (NGC 628, NGC 783, NGC 2336, NGC 6217, NGC 6946, NGC 7331, and NGC 7678). The complete observational database has been observed and accumulated within the framework of our comprehensive study of extragalactic star forming regions. The current paper presents the last part of either unpublished or refreshed photometric and spectrophotometric observations of the galaxies NGC 6217, NGC 6946, NGC 7331, and NGC 7678. We derive extinctions, chemical abundances, continuum and line emissions of ionised gas, ages and masses for cluster complexes. We find the young massive cluster complexes to have ages no greater than 10 Myr and masses between 10^4Msol and 10^7Msol, and the extinctions A(V) vary between ~ 0 and 3 mag, while the impact of the nebular emission on integrated broadband photometry mainly is not greater than 40% of the total flux and is comparable with accuracies of dereddened photometric quantities.We also find evidence of differential extinction of stellar and gas emissions in some clusters, which hinders the photometric determination of ages and masses in these cases. Finally, we show that young massive cluster complexes in the studied galaxies and open clusters in the Milky Way form a continuous sequence of luminosities/masses and colour/ages.