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Young Massive Star Clusters [PDF]

open access: yesAnnual Review of Astronomy and Astrophysics, 2010
Young massive clusters (YMCs) are dense aggregates of young stars that form the fundamental building blocks of galaxies. Several examples exist in the Milky Way Galaxy and the Local Group, but they are particularly abundant in starburst and interacting galaxies.
Zwart, SP, McMillan, S, Gieles, M
openaire   +4 more sources

Young Star Clusters in M 31 [PDF]

open access: yes, 2008
In our study of M31's globular cluster system with MMT/Hectospec, we have obtained high-quality spectra of 85 clusters with ages less than 1 Gyr. With the exception of Hubble V, the young cluster in NGC 205, we find that these young clusters have kinematics and spatial distribution consistent with membership in M31's young disk.
Morrison, Heather   +5 more
openaire   +3 more sources

Young Star Clusters: Progenitors of Globular Clusters!? [PDF]

open access: yesHighlights of Astronomy, 2005
AbstractStar cluster formation is a major mode of star formation in the extreme conditions of interacting galaxies and violent starbursts. Young clusters are observed to form in a variety of such galaxies, a substantial number resembling the progenitors of globular clusters in mass and size, but with significantly enhanced metallicity.
Anders, Peter   +2 more
openaire   +3 more sources

Young Star Clusters in the LMC [PDF]

open access: yesSymposium - International Astronomical Union, 1991
We discuss the integrated colours, kinematics, formation, dynamical evolution and initial mass functions of the young globular star clusters in the Large Magellanic Cloud (LMC). Because these clusters are so young, they offer us insights, unobtainable from the old globular clusters in our Galaxy, into the formation and early dynamical evolution of ...
K. C. Freeman, R.A.W. Elson
openaire   +1 more source

Be Stars in Young LMC Clusters [PDF]

open access: yesSymposium - International Astronomical Union, 1994
Slitless field Hα spectroscopy with a resolution of 0.2 nm has detected numerous Be stars in 3 young open star clusters in the LMC but only a few each in one Galactic and one LMC cluster. The line widths indicate rapid rotation as is typical of Galactic field Be stars.
H. Kjeldsen, D. Baade
openaire   +1 more source

Multi-Color Observations of Young Star Clusters [PDF]

open access: yesHighlights of Astronomy, 2005
AbstractWe present a new set of evolutionary synthesis models of our GALEV code, specifically developed to include the gaseous emission of presently forming star clusters, in combination with an advanced tool to compare large model grids with multi-color broad-band observations of YSC systems. Tests and first applications are presented.
Anders, Peter   +2 more
openaire   +3 more sources

THE BRIGHTEST YOUNG STAR CLUSTERS IN NGC 5253 [PDF]

open access: yesThe Astrophysical Journal, 2015
67 pages; 11 figures; 7 tables.
Calzetti, D.   +46 more
openaire   +9 more sources

Star formation in young star cluster NGC 1893 [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2007
We present a comprehensive multi-wavelength study of the star-forming region NGC 1893 to explore the effects of massive stars on low-mass star formation. Using near-infrared colours, slitless spectroscopy and narrow-band $H $ photometry in the cluster region we have identified candidate young stellar objects (YSOs) distributed in a pattern from the ...
Sharma, Saurabh   +8 more
openaire   +3 more sources

Young star clusters in nearby molecular clouds [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2018
Accepted for publication in MNRAS (on February 19, 2018); 30 pages, 14 figures, and 8 ...
K V Getman   +5 more
openaire   +3 more sources

Dynamics of black hole–neutron star binaries in young star clusters [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2020
ABSTRACT Young star clusters are likely the most common birthplace of massive stars across cosmic time and influence the formation of compact binaries in several ways. Here, we simulate the formation of black hole–neutron star binaries (BHNSs) in young star clusters, by means of the binary population synthesis code MOBSE interfaced with ...
Sara Rastello   +7 more
openaire   +3 more sources

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