Results 121 to 130 of about 106,016 (255)
Progressive Star Formation in the Young SMC Cluster NGC 602 [PDF]
L. R. Carlson +11 more
openalex +1 more source
The Stellar Initial Mass Function of Early Dark Matter–free Gas Objects
Among the remarkable strides made by JWST is the discovery of the earliest star clusters found to date. These have been proposed as early progenitors of globular clusters, which are known to come from the early stages of star formation in the Universe ...
William Lake +8 more
doaj +1 more source
AChandraX-ray study of the young star cluster NGC 6231: low-mass population and initial mass function [PDF]
F. Damiani, G. Micela, S. Sciortino
openalex +1 more source
Fast-rotating A- and F-type Stars with Hα Emissions in NGC 3532: Candidate UV-dim Stars?
Extended main-sequence stars that are dim in the ultraviolet passbands of the Hubble Space Telescope (UV-dim stars) are found in several young and intermediate-age star clusters in the Magellanic Clouds (MCs).
Chenyu He, Chengyuan Li, Gang Li
doaj +1 more source
The mass function of young star clusters in spiral galaxies [PDF]
S. S. Larsen
openalex +1 more source
Red supergiants (RSGs) represent a late evolutionary stage of massive stars. Recent observations reveal that the observed luminosity range of RSGs in young open clusters is wider than expected from single-star evolution models.
Chen Wang +14 more
doaj +1 more source
Super star clusters in Haro 11: properties of a very young starburst and evidence for a near-infrared flux excess [PDF]
Angela Adamo +5 more
openalex +1 more source
Young star cluster evolution and metallicity
2 pages, 1 figure, to appear in Stellar Populations 55 years after the Vatican conference, Proceedings of the Symposium 6 of the European Week of Astronomy and Space Science 2012 (EWASS 2012), held July 2-4, 2012 in Roma, Italy.
Mapelli, M., Bressan, A.
openaire +3 more sources
Disk-locking Regulates Stellar Rotation in Young Clusters: Insights from NGC 2264
Many young clusters possess extended main sequences, a phenomenon commonly ascribed to stellar rotation. However, the mechanism behind their very wide stellar rotation distributions remains unclear.
Yutian Bu +3 more
doaj +1 more source

