Results 211 to 220 of about 274,405 (356)
THE YOUNG, MASSIVE, STAR CLUSTER SANDAGE-96 AFTER THE EXPLOSION OF SUPERNOVA 2004dj IN NGC 2403 [PDF]
J. Vinkó+14 more
openalex +1 more source
The young massive stellar cluster Westerlund 1 in gamma rays as seen with H.E.S.S. [PDF]
L. Mohrmann+4 more
openalex +1 more source
eChem: Accelerated Method Development in Quantum Chemistry with Notebooks
The benefits of using Jupyter Notebooks to simplify and accelerate scientific code development are demonstrated using the practical example of the analytical molecular Hessian. The eChem project has been previously presented as an interactive platform for quantum and computational chemistry education [J. Chem. Educ. 100, 1664–1671].
Manuel Hodecker+2 more
wiley +1 more source
Pre-main-sequence stars in the young open cluster NGC 1893 II. Evidence for triggered massive star formation [PDF]
I. Negueruela+3 more
openalex +1 more source
Tsunami events over the past 500 years inundated Laguna Gemela West (Chile), leading to distinct sandy deposits in the lake record. This provides a complete perspective on tsunami inundation, including giant tsunamis, small local tsunamis and tsunamis that originated >100 km away from the site.
Jasper Moernaut+8 more
wiley +1 more source
Young Massive Star Clusters in Normal Galaxies
8 pages, invited contribution for the Cancun Workshop on Formation and Evolution of Young Massive Clusters, eds. H. J. G. L. M. Lamers, A.
openaire +2 more sources
Shallow‐marine mudstone of the Cretaceous Kaskapau Formation in the British Columbia foredeep preserves a 185 m thick record of OAE2. The organic carbon‐isotope and osmium‐isotope excursions can be correlated in detail with other Cenomanian–Turonian boundary sections around the world.
A. Guy Plint+12 more
wiley +1 more source
Discovery of a young and massive stellar cluster [PDF]
S. Ramírez Alegría+2 more
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Controls on carbonate island formation and evolution: South Joulter Cay, Great Bahama Bank
The evolution of South Joulter Cay occurs in three stages: linear ridges shaped by waves and longshore currents, arcuate ridges influenced by tidal currents and channels, and cuspate ridges formed by variable wind and wave directions. These processes are driven by climatic and oceanographic factors.
Juan Carlos Laya+3 more
wiley +1 more source
Young Massive Clusters as probes of stellar evolution
Young Massive Clusters (YMCs) represent ideal testbeds in which to study massive stellar evolution as they contain large, coeval, chemically homogeneous, samples of massive stars. By studying YMCs with a range of ages (and hence turn-off masses), we can investigate the post main-sequence evolution of massive stars as a function of initial mass.
openaire +2 more sources