The Astrophysical JournalEffectively finding and identifying active galactic nuclei (AGNs) in dwarf galaxies is an important step in studying black hole formation and evolution.
Megan R. Sturm +2 more
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Extended main sequences in star clusters
Fundamental ResearchExtended main sequences (eMSs) and extended main-sequence turn-offs (eMSTOs) are fascinating phenomena that are routinely observed in star clusters. These phenomena strongly challenge the current canonical “simple stellar population” picture of star ...
Chengyuan Li +3 more
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CLOSE STELLAR ENCOUNTERS IN YOUNG, SUBSTRUCTURED, DISSOLVING STAR CLUSTERS: STATISTICS AND EFFECTS ON PLANETARY SYSTEMS [PDF]
, 2013 Jonathan Craig, Mark R. Krumholz
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Dynamical formation of $Gaia$ BH1 in a young star cluster [PDF]
, 2023 Sara Rastello +7 more
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STELLAR FEEDBACK IN MOLECULAR CLOUDS AND ITS INFLUENCE ON THE MASS FUNCTION OF YOUNG STAR CLUSTERS [PDF]
, 2010 S. Michael Fall +2 more
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Cosmic Ray Enrichment with 22Ne in Young Massive Star Clusters [PDF]
, 2023 M. E. Kalyashova +2 more
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Topography of the Young Galactic Disk: Spatial and Kinematic Patterns of Clustered Star Formation in the Solar Neighborhood [PDF]
, 2022 E. J. Alfaro +5 more
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Young Star Clusters in Starburst Environments
, 1996 Recent high-resolution observations with the Hubble Space Telescope (HST) reveal that young star clusters of extraordinary luminosity and compactness ("super star clusters") are commonly found in starburst systems. Cluster formation appears to be a dominant mode of star formation in starbursts.
openaire +2 more sources
Identification of Outer Galaxy Cluster Members Using Gaia DR3 and Multidimensional Simulation
The Astronomical JournalThe outer Galaxy presents a distinctive environment for investigating star formation. This study develops a novel approach to identify true cluster members based on unsupervised clustering using astrometry with significant uncertainties.
Vishwas Patel +3 more
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Massive Clusters and OB Associations as Output of Massive Star Formation in Gaia Era
UniverseOver the past two decades, our understanding of star formation has undergone a major shift, driven by a wealth of data from infrared, submillimeter and radio surveys. The emerging view depicts star formation as a hierarchical process, which predominantly
Ignacio Negueruela
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