Results 111 to 120 of about 4,118,940 (288)
The obscured hyper-energetic GRB 120624B hosted by a luminous compact galaxy at z=2.20 [PDF]
, 2013 Context. Gamma-ray bursts (GRBs) are the most luminous explosions that we can witness in the Universe. Studying the most extreme cases of these phenomena allows us to constrain the limits for the progenitor models. Aims.
de Ugarte Postigo, A. +35 more
core +1 more source
Interstellar medium properties and star formation in nearby galaxies [PDF]
, 2014 Includes bibliographical references.We study the properties of the interstellar medium (ISM) of nearby galaxies from The HI Nearby Galaxy Survey (THINGS) by analyzing the shapes of their HI emission velocity profiles.
Ianjamasimanana, Roger
core +1 more source
The Momentum of ‘Developed’: Bodies of Water, Aging Bodies and Malta's Interventions at the UN
History, EarlyView.Abstract Histories of major powers continue to shape how many scholars conceptualize internationalism. By focusing on Malta's interventions at the UN challenges, this article challenges such narrative. In particular, it examines Arvid Pardo's 1967 petition that the seabed be reconceived and protected as the ‘common heritage of mankind’ and Vincent ...
Brianne Wesolowski
wiley +1 more source
Origin and Evolution of Large-scale Magnetic Fields [PDF]
, 2015 Magnetic elds are ubiquitous at all scales in the Universe and have been observed in galaxies and clusters of galaxies via observations of di use radio emission and Faraday Rotation Measures.
Barnes, DJ
core
International Journal of Urban and Regional Research, EarlyView.Abstract In terms of mainstream sustainability economics, market‐led initiatives aimed at biodiversity restoration represent a productive, morally conscientious choice. Under this view, efforts in areas such as biodiversity offsetting, net gain, or finance are considered effective tools for preventing or managing environmental degradation.
Ihnji Jon
wiley +1 more source
Integral-Field Spectroscopy of High-Redshift Galaxies: Implications for Early Galaxy Evolution [PDF]
, 2006 Several lines of evidence suggest that the most active phase of galaxy evolution, especially in the most massive systems, was largely completed by $z\sim 1$.
Nesvadba, Nicole
core +1 more source
TNG SAM: Bridging Hydrodynamical Complexity and Semianalytic Efficiency to Model Galaxy Formation
The Astrophysical JournalAll cosmological models of galaxy formation must navigate the trade-off between physical accuracy and computational efficiency. Hydrodynamical simulations provide spatially resolved predictions for the coevolution of dark matter, gas, stars, and black ...
Osase Omoruyi +7 more
doaj +1 more source
Insect Science, EarlyView.The Australian giant wood moth (Endoxyla cinereus) feeds within the galls of scale insects (Apiomorpha) before transitioning into its wood‐boring eucalypt larval phase. This transitionary phase may be key to its multi‐year development, at the end of which it can produce over 100 000 eggs.
Jessa H. Thurman +4 more
wiley +1 more source
Measuring the star formation rate density from CNOC2 [PDF]
, 2006 This thesis charts the evolution of the Universal Star Formation Rate Density (SFRD) across the redshift range 0.2 < z < 0.6, using the 2nd Canadian Network for Observational Cosmology Survey (CN0C2).
Whitaker, Richard James
core
Gas, star formation and quenching in galaxy clusters and groups [PDF]
, 2019 I will review our current knowledge of the link between the star formation activity+quenching and the gas availability and removal as a function of galaxy environment focusing on galaxy clusters and groups.
POGGIANTI, Bianca Maria +1 more
core +1 more source