Results 111 to 120 of about 593,443 (246)
Modelling galaxy stellar mass evolution from z~0.8 to today
, 2009 We apply the empirical method built for z=0 in the previous work of Wang et al. to a higher redshift, to link galaxy stellar mass directly with its hosting dark matter halo mass at z~0.8.
Jing, Y. P., Wang, Lan
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Clusters of Galaxies as Storage Room for Cosmic Rays [PDF]
, 1997 V. Berezinsky +2 more
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SPITZER POINT-SOURCE CATALOGS OF ~ 300,000 STARS IN SEVEN NEARBY GALAXIES [PDF]
, 2015 Rubab Khan +3 more
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Dense Molecular Gas Associated with the Circumnuclear Star‐forming Ring in the Barred Spiral Galaxy NGC 6951 [PDF]
, 1999 Kotaro Kohno +2 more
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Metagenomic analysis of goat feces from Ogliastra (Sardinia, Italy)
Frontiers in MicrobiomesWith its constitutive and functional characteristics, the intestinal microbiota plays a crucial role in the health condition of the animals. Variations in the composition and gene expression of the intestinal microbiota are associated with the risk of ...
Monica Rosaria Molotzu +5 more
doaj +1 more source
, 2006 In a Lambda CDM Universe, galaxies grow in mass both through star formation and through addition of already-formed stars in galaxy mergers. Because of this partial decoupling of these two modes of galaxy growth, I discuss each separately in this biased and incomplete review of galaxy assembly; first giving an overview of the cosmic-averaged star ...
openaire +2 more sources
, 2013 Galaxy morphology is a product of how galaxies formed, how they interacted with their environment, how they were influenced by internal perturbations, AGN, and dark matter, and of their varied star formation histories. This article reviews the phenomenology of galaxy morphology and classification with a view to delineating as many types as possible and
openaire +3 more sources
Slim Disks with Transition Regions and Applications to Microquasars and Narrow‐Line Seyfert 1 Galaxies [PDF]
, 2004 Lin‐Hong Chen, Jian‐Min Wang
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Disk Galaxies and Galaxy Disks
, 2000 The conference Galaxy Disks and Disk Galaxies, sponsored by the Vatican Observatory, was held in June 12-16, 2000 at the Pontifical Gregorian University, in Rome (Italy). The meeting hosted about 230 participants coming from 30 countries. The very full program consisted of 29 review papers, 34 invited talks, and more than 180 posters.
J, J. G. Funes S., Corsini, E. M.
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, 2022 Galaxy clusters grow by accreting galaxies from the field and along filaments of the cosmic web. As galaxies are accreted they are affected by their local environment before they enter (pre-processing), and traverse the cluster potential. Observations that aim to constrain pre-processing are challenging to interpret because filaments comprise a ...
Kuchner, Ulrike +6 more
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