Results 21 to 30 of about 180,283 (246)
Probing the Physics of Interacting Galaxies
Astrophysics and Space Science, 2003 Both Arp 140 and Arp 104 reveal extended tidal tails in the HI. The Halpha and FIR fluxes of Arp 140 yield similar SFR of ~0.8 solar masses per year. In contrast the Halpha flux of Arp 104 yields a SFR of ~0.05 solar masses per year, ~ 20 times smaller than that obtained from the FIR flux.
Cullen, Harriet +2 more
openaire +2 more sources
Statistical Inconsistencies in the KiDS-450 Dataset [PDF]
, 2017 The Kilo-Degree Survey (KiDS) has been used in several recent papers to infer constraints on the amplitude of the matter power spectrum and matter density at low redshift. Some of these analyses have claimed tension with the Planck $\Lambda \mathrm{CDM}$
Efstathiou, George, Lemos, Pablo
core +2 more sources
Targeted decrease of portal hepatic pressure gradient improves ascites control after TIPS
Hepatology, EarlyView., 2022 The river diagram demonstrates that after transjugular intrahepatic portosystemic shunt insertion (TIPS) the majority of patients without ascites and 50% of the patients with ascites detectable at ultrasound, show the best response in the long term follow‐up.
Alexander Queck +14 more
wiley +1 more source
The physics of galaxy evolution with EAGLE [PDF]
1st AO4ELT conference - Adaptive Optics for Extremely Large Telescopes, 2010 6 pages, 4 Figures, to appear in the proceedings of the AO4ELT meeting held in Paris, 22-26 June ...
Puech, Mathieu +9 more
openaire +4 more sources
The Open Journal of Astrophysics, 2023 The recent launch of JWST has ushered in a new era of high-redshift astronomy by providing detailed insights into the gas and stellar populations of galaxies in the epoch of reionization.
Harley Katz +9 more
doaj +1 more source
Can simulations reproduce the observed temperature-mass relation for clusters of galaxies? [PDF]
, 2001 It has become increasingly apparent that traditional hydrodynamical simulations of galaxy clusters are unable to reproduce the observed properties of galaxy clusters, in particular overpredicting the mass corresponding to a given cluster temperature ...
Afshordi +33 more
core +4 more sources
Physical Morphology of Galaxies using Asymmetry [PDF]
Astrophysics and Space Science, 1999 We demonstrate in this paper the use of asymmetry in conjunction with the integrated (B-V) color of galaxies for physical morphological purposes. We show how color-asymmetry diagrams can be used to distinguish between various types of galaxies, including ellipticals, late and early type disks, irregulars and interacting/merging galaxies.
openaire +2 more sources
Physical Classification of Galaxies with MOPED∕VESPA [PDF]
AIP Conference Proceedings, 2008 Invited talk at the class2008 meeting in ...
Raul Jimenez +4 more
openaire +3 more sources
Physical Properties and Environments of Nearby Galaxies [PDF]
Annual Review of Astronomy and Astrophysics, 2009 We review the physical properties of nearby, relatively luminous galaxies, using results from newly available massive data sets together with more detailed observations. First, we present the global distribution of properties, including the optical and ultraviolet (UV) luminosity, stellar mass, and atomic gas mass functions.
Blanton, Michael R., Moustakas, John
openaire +2 more sources
LoCuSS: Probing galaxy transformation physics withHerschel [PDF]
Astronomy and Astrophysics, 2010 5 pages, 4 figures, accepted for publication by A&A ...
Smith, G. +14 more
openaire +3 more sources