Galactic Rotation from Young Open Star Clusters [PDF]
The rotation of the Galaxy can best be studied with the aid of tracers for which distance and velocity can be obtained simultaneously, accurately and unambiguously out to large distances. Clearly, the best objects are the very young clusters. The local gradient of the angular velocity is contained in Oort's constant and, due e.g. to perturbations from
H. M. Maitzen +2 more
openaire +1 more source
Constraining the Fraction of Binary Black Holes Formed in Isolation and Young Star Clusters with Gravitational-wave Data [PDF]
Ten binary black hole mergers have already been detected during the first two observing runs of advanced LIGO and Virgo, and many more are expected to be observed in the near future.
Y. Bouffanais +6 more
semanticscholar +1 more source
The Cosmic Evolution of Binary Black Holes in Young, Globular and Nuclear Star Clusters: Rates, Masses, Spins and Mixing Fractions [PDF]
The growing population of binary black holes (BBHs) observed by gravitational wave detectors is a potential Rosetta stone for understanding their formation channels. Here, we use an upgraded version of our semi-analytic codes fastcluster and cosmoRate to
M. Mapelli +4 more
semanticscholar +1 more source
GW190521 formation via three-body encounters in young massive star clusters [PDF]
GW190521 is the most massive binary black hole (BBH) merger observed to date, and its primary component lies in the pair-instability (PI) mass gap. Here, we investigate the formation of GW190521-like systems via three-body encounters in young massive ...
Marco Dall’Amico +7 more
semanticscholar +1 more source
The young Galactic star cluster [DBS2003] 179 [PDF]
Recent near- and mid-infrared surveys have brought evidence that the Milky Way continues to form massive clusters. We carry out a program to determine the basic physical properties of the new massive cluster candidate [DBS2003]179. Medium-resolution K-band spectra and deep near-infrared images of [DBS2003]179 were used to derive the spectral types of ...
Borissova, J. +6 more
openaire +3 more sources
Discrepancies in the ages of young star clusters; evidence for mergers? [PDF]
There is growing evidence that star clusters can no longer be considered simple stellar populations (SSPs). Intermediate and old age clusters are often found to have extended main sequence turn-offs (eMSTOs) which are difficult to explain with single age
Emma R. Beasor +3 more
semanticscholar +1 more source
Effects of Close Binary Evolution on the Main-sequence Morphology of Young Star Clusters [PDF]
Star clusters are the building blocks of galaxies. They are composed of stars of nearly equal age and chemical composition, allowing us to use them as chronometers and as testbeds for gauging stellar evolution.
Chen Wang +6 more
semanticscholar +1 more source
Universal Upper End of the Stellar Initial Mass Function in the Young and Compact LEGUS Clusters
We investigate the variation in the upper end of the stellar initial mass function (uIMF) in 375 young and compact star clusters in five nearby galaxies within ∼5 Mpc. All the young stellar clusters (YSCs) in the sample have ages ≲ 4 Myr and masses above
Dooseok Escher Jung +23 more
doaj +1 more source
Connecting young star clusters to CO molecular gas in NGC 7793 with ALMA–LEGUS [PDF]
We present an investigation of the relationship between giant molecular cloud (GMC) properties and the associated stellar clusters in the nearby flocculent galaxy NGC 7793. We combine the star cluster catalogue from the HST LEGUS (Legacy ExtraGalactic UV
K. Grasha +24 more
semanticscholar +1 more source
The public, all-sky surveys Gaia and TESS provide the ability to identify new young associations and determine their ages. These associations enable study of planetary evolution by providing new opportunities to discover young exoplanets.
Elisabeth R. Newton +38 more
doaj +1 more source

