Results 31 to 40 of about 2,879,280 (414)

Simultaneous Estimates of Star-cluster Age, Metallicity, Mass, and Extinction (SESAMME). I. Presenting an MCMC Approach to Spectral Stellar Population Fitting

open access: yesThe Astrophysical Journal, 2023
We present the first version release of SESAMME, a public, Python-based full spectrum fitting tool for Simultaneous Estimates of Star-cluster Age, Metallicity, Mass, and Extinction.
Logan H. Jones   +5 more
doaj   +1 more source

The E-MOSAICS project: simulating the formation and co-evolution of galaxies and their star cluster populations [PDF]

open access: yes, 2017
We introduce the MOdelling Star cluster population Assembly In Cosmological Simulations within EAGLE (E-MOSAICS) project. E-MOSAICS incorporates models describing the formation, evolution, and disruption of star clusters into the EAGLE galaxy formation ...
J. Pfeffer   +3 more
semanticscholar   +1 more source

Bruck 88 : a young star cluster with an old age resemblance in the outskirts of the Small Magellanic Cloud [PDF]

open access: yes, 2014
We present spectroscopic and photometric results for the Small Magellanic Cloud (SMC) cluster Bruck 88. From the comparison of the cluster integrated spectrum with template cluster spectra we found that the Milky Way globular cluster template spectra are
Piatti, Andrés E.
core   +3 more sources

Sub-clinical abnormalities detected by PET/MRI in household tuberculosis contacts

open access: yesBMC Infectious Diseases, 2019
Background The understanding of early events following TB exposure is limited by traditional tests that rely on detection of an immune response to infection, which is delayed, or on imaging tests with low sensitivity for early disease.
James S. Molton   +11 more
doaj   +1 more source

Molecular Gas Properties in Young Stellar Clusters with a Suppressed Star Cluster Wind

open access: yesThe Astrophysical Journal Letters, 2023
In compact and dense star-forming clouds a global star cluster wind could be suppressed. In this case stellar feedback is unable to expel the leftover gas from the cluster. Young massive stars remain embedded in a dense residual gas and stir it by moving
Sergiy Silich   +3 more
doaj   +1 more source

The R136 star cluster dissected with Hubble Space Telescope/STIS. I. Far-ultraviolet spectroscopic census and the origin of He II λ1640 in young star clusters [PDF]

open access: yes, 2016
We introduce a Hubble Space Telescope (HST)/Space Telescope Imaging Spectrograph (STIS) stellar census of R136a, the central ionizing star cluster of 30 Doradus.
P. Crowther   +19 more
semanticscholar   +1 more source

The Star Formation History of the Milky Way’s Nuclear Star Cluster

open access: yesThe Astrophysical Journal, 2023
We report the first star formation history study of the Milky Ways nuclear star cluster (NSC), which includes observational constraints from a large sample of stellar metallicity measurements.
Zhuo Chen   +8 more
doaj   +1 more source

Orbital Decay and Tidal Disruption of a Star Cluster: Analytical Calculation [PDF]

open access: yes, 2002
The orbital decay and tidal disruption of a star cluster in a galaxy is studied in an analytical manner. Owing to dynamical friction, the star cluster spirals in toward the center of the galaxy.
Fall S. M.   +4 more
core   +2 more sources

Identification of small molecules targeting homoserine acetyl transferase from Mycobacterium tuberculosis and Staphylococcus aureus

open access: yesScientific Reports, 2022
There is an urgent need to validate new drug targets and identify small molecules that possess activity against both drug-resistant and drug-sensitive bacteria.
Deepika Chaudhary   +13 more
doaj   +1 more source

Star cluster formation in a turbulent molecular cloud self-regulated by photoionization feedback [PDF]

open access: yes, 2017
Most stars in the Galaxy are believed to be formed within star clusters from collapsing molecular clouds. However, the complete process of star formation, from the parent cloud to a gas-free star cluster, is still poorly understood.
E. Gavagnin   +3 more
semanticscholar   +1 more source

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