WIDE-FIELD INFRARED SURVEY EXPLORER OBSERVATIONS OF THE EVOLUTION OF MASSIVE STAR-FORMING REGIONS

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Feedback from winds and supernovae in massive stellar clusters – I. Hydrodynamics (2012, background): “…likely inhibit further star formation as their winds and ionizing radiation disperse and destroy the remaining molecular gas, though in some circumstances massive stars may also trigger new star formation (Koenig et al. 2012) and new cluster formation (Beuther et al. 2008; Gray & Scannapieco 2011).”
The WISE AGN Catalog (2017, background): “Some of them can be, for example, YSOs and AGB stars, which have similar colors to AGN in the WISE bands (see, e.g., Koenig et al. 2012; Nikutta et al. 2014).”
Modeling UV Radiation Feedback from Massive Stars. II. Dispersal of Star-forming Giant Molecular Clouds by Photoionization and Radiation Pressure (2018, background): “…map is dominated by bright, compact H II regions around newly formed stars, while at later times it becomes rich in substructures resembling observed pillars and bright-rimmed globules (e.g., Koenig et al. 2012; Hartigan et al. 2015); these features are also apparent in the ne slices of Figure 3.”