Results 31 to 40 of about 438,137 (232)

STROMGREN PHOTOMETRY AND SEARCH FOR SHORT PERIOD VARIABLES IN THE OPEN CLUSTERS NGC 6910 AND NGC 6913

open access: yesOdessa Astronomical Publications, 2017
Analysis of the absolute uvby photometry of the Open Clusters NGC 6910 and NGC 6913 show well-defined peaks that clearly define the accumulation of stars. Differential photometry of five stars in the direction of each cluster determines that at least two
J. H. Pena   +5 more
doaj   +1 more source

Star cluster formation and star formation: the role of environment and star-formation efficiencies [PDF]

open access: yes, 2008
“The original publication is available at www.springerlink.com”. Copyright Springer. DOI: 10.1007/s10509-009-0088-5By analyzing global starburst properties in various kinds of starburst and post-starburst galaxies and relating them to the properties of ...
A. Pasquali   +58 more
core   +2 more sources

Early Results from GLASS-JWST. XX. Unveiling a Population of “Red Excess” Galaxies in Abell2744 and in the Coeval Field

open access: yesThe Astrophysical Journal Letters, 2023
We combine JWST/NIRCam imaging and MUSE data to characterize the properties of galaxies in different environmental conditions in the cluster Abell2744 ( z = 0.3064) and in its immediate surroundings. We investigate how galaxy colors, morphology, and star-
Benedetta Vulcani   +28 more
doaj   +1 more source

Star Cluster Survival in Star Cluster Complexes under Extreme Residual Gas Expulsion

open access: yes, 2005
After the stars of a new, embedded star cluster have formed they blow the remaining gas out of the cluster. Especially winds of massive stars and definitely the on-set of the first supernovae can remove the residual gas from a cluster.
Baumgardt H.   +3 more
core   +2 more sources

Survey for Distant Stellar Aggregates in the Galactic Disk: Detecting 2000 Star Clusters and Candidates, along with the Dwarf Galaxy IC 10

open access: yesThe Astrophysical Journal Supplement Series, 2023
Despite having data for over 10 ^9 stars from Gaia, less than 10 ^4 star clusters and candidates have been discovered. In particular, distant star clusters are rarely identified, due to the challenges posed by heavy extinction and great distance. However,
Zhihong He   +7 more
doaj   +1 more source

How star clusters could survive low star formation efficiencies

open access: yes, 2004
After the stars of a new, embedded star cluster have formed they blow the remaining gas out of the cluster. Especially winds of high mass stars and definitely the on-set of the first super novae can remove the residual gas from a cluster. This leads to a
Fellhauer, M., Kroupa, P.
core   +1 more source

Star Formation History of a Young Super-Star Cluster in NGC 4038/39: Direct Detection of Low Mass Pre-Main Sequence Stars [PDF]

open access: yes, 2010
We present an analysis of the near-infrared spectrum of a young massive star cluster in the overlap region of the interacting galaxies NGC 4038/39 using population synthesis models.
Blum   +34 more
core   +2 more sources

The role of the central stellar cluster in active galactic nuclei. I. Semi-analytical model [PDF]

open access: yes, 2002
The subject of the paper is the role of the massive stellar cluster in the activity phenomenon and in the structure of active galactic nuclei. We introduce a simple model of stellar dynamics in the internal part of the cluster, which allows us to include
Czerny, B., Vilkoviskij, E. Y.
core   +2 more sources

Cluster and Double Star observations of dipolarization [PDF]

open access: yesAnnales Geophysicae, 2005
We studied two types of dipolarization events with different IMF conditions when Cluster and Double Star (TC-1) were located in the same local time sector: 7 August 2004, 18:00-24:00 UT, during a disturbed southward/northward IMF interval, and 14
R. Nakamura   +18 more
doaj   +1 more source

Probing embedded star clusters in the HII complex NGC 6357 with VVV [PDF]

open access: yes, 2014
NGC 6357 is an active star-forming region located in the Sagittarius arm displaying several star clusters, which makes it a very interesting target to investigate star formation and early cluster evolution.
Bica, E.   +3 more
core   +3 more sources

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