Results 141 to 150 of about 1,140 (187)
Possible nonstellar explanation for the unexpected brightness of the earliest galaxies observed by the James Webb Space Telescope. [PDF]
Jacak JE.
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A decade of sub-arcsecond imaging with the International LOFAR Telescope. [PDF]
Morabito LK +9 more
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A luminous and young galaxy at z = 12.33 revealed by a JWST/MIRI detection of Hα and [O iii]. [PDF]
Zavala JA +39 more
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Primordial Rotating Disk Composed of ≥15 Star Forming Clumps at Cosmic Dawn
Fujimoto S +45 more
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Cosmology and astrophysics with galaxy clusters
AIP Conference Proceedings, 2014Galaxy clusters are the largest gravitationally bound objects in the universe, whose formation is driven by dark energy and dark matter. The majority of the baryonic mass in clusters resides in the hot X-ray emitting plasma, which also leaves imprints in the cosmic microwave background radiation.
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The Molecular Astrophysics of Stars and Galaxies
1998Abstract This book provides a comprehensive survey of modern molecular astrophysics. It includes an introduction to molecular spectroscopy and then addresses the main areas of current molecular astrophysics, including galaxy formation, star forming regions, mass loss from young as well as highly evolved stars and supernovae, starburst
Thomas W Hartquist, David A Williams
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Enhanced cobweb clustering for identifying analog galaxies in astrophysics
2014 IEEE 27th Canadian Conference on Electrical and Computer Engineering (CCECE), 2014Clustering, a very popular task in Data Mining, is unsupervised classification of patterns (observations, data items, or feature vectors) into groups (clusters). Clustering has been explored in many different contexts and disciplines. In this paper, we explore using the COBWEB clustering algorithm to identify and group together galaxies whose spectral ...
Ashwin Satyanarayana, Viviana Acquaviva
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The Multifrequency Astrophysics of Galaxy Clusters
Chinese Journal of Astronomy and Astrophysics, 2003We discuss the evidence and the physical relevance of the astrophysical phenomena (of thermal and non-thermal origin) occurring in galaxy clusters as obtained from multi-frequency observations, from radio to gamma-rays.
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