Results 1 to 10 of about 314 (90)

Made-to-measure galaxy models - II Elliptical and Lenticular Galaxies [PDF]

open access: yesRoyal Astronomical Society. Monthly Notices, 2012
14 pages, 8 figures and 5 ...
Long, R. J., Mao, Shude
core   +4 more sources

The SAURON project - X. The orbital anisotropy of elliptical and lenticular galaxies [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2007
We analyse the orbital distribution of elliptical (E) and lenticular (S0) galaxies using SAURON integral-field stellar kinematics within about one effective (half-light) radius. We construct the anisotropy diagram, which relates the ratio of the ordered and random motion in a galaxy (V/sigma) to its observed ellipticity (epsilon), for the 48 E/S0 ...
Cappellari, Michele   +13 more
core   +6 more sources

The Invisibility of Scotomas I: The Carving Hypothesis

open access: yesOptometry and Vision Science, Volume 100, Issue 8, Page 515-529, August 2023., 2023
SIGNIFICANCE Veridical depictions of scene appearance with scotomas allow better understanding of the impact of field loss and may improve the development and implementation of rehabilitation. Explanation and depiction of the invisibility of scotoma may lead to patients' understanding and thus better compliance with related treatments.
Eli Peli   +2 more
wiley   +1 more source

The colour-magnitude relation of Elliptical and Lenticular galaxies in the ESO Distant Cluster Survey [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2008
14 pages, 12 figures, accepted for publication in ...
Jaffé Y. L   +6 more
openaire   +4 more sources

Comparison between a handheld ultrasound device and a traditional ultrasound for performing transcranial sonography in patients with Parkinson's disease

open access: yesBrain and Behavior, Volume 13, Issue 2, February 2023., 2023
Graph 1. The receiver operating characteristic (ROC) curve. The area under the curve is 0.91 with a confidence interval (CI) of 95%: 0.84–0.97. The best substantia nigra cutoff value was 0.20 cm2. Sensitivity = 0.98 and specificity = 0.87. Abstract Objective The aim of this study is to compare a portable ultrasound (US) device and a traditional US for ...
Maria A. S. Paes   +5 more
wiley   +1 more source

The role of siliciclastics in carbonate fabric diversity and preservation: A case study from the Neoproterozoic carbonate − siliciclastic Horse Thief Springs Formation, Death Valley

open access: yesSedimentology, Volume 69, Issue 5, Page 2284-2318, August 2022., 2022
Abstract The sedimentary record of the Pahrump Group in Death Valley comprises well‐exposed successions of mixed carbonate and siliciclastic deposits. Despite the abundance of studies focussing on the depositional dynamics of mixed carbonate – siliciclastic deposition in the Phanerozoic, the record of similar Proterozoic examples is comparatively ...
Daniel Smrzka   +7 more
wiley   +1 more source

Compact elliptical galaxies – compact bulges of stripped lenticulars/spirals? [PDF]

open access: yesProceedings of the International Astronomical Union, 2007
AbstractWe present discovery of compact elliptical galaxies in the centres of clusters and briefly discuss their evolution.
Chilingarian, Igor V.   +3 more
openaire   +1 more source

Bose‐Einstein Condensate Dark Matter Halos Confronted with Galactic Rotation Curves

open access: yesAdvances in High Energy Physics, Volume 2017, Issue 1, 2017., 2017
We present a comparative confrontation of both the Bose‐Einstein Condensate (BEC) and the Navarro‐Frenk‐White (NFW) dark halo models with galactic rotation curves. We employ 6 High Surface Brightness (HSB), 6 Low Surface Brightness (LSB), and 7 dwarf galaxies with rotation curves falling into two classes.
M. Dwornik   +4 more
wiley   +1 more source

The Study of Nebular Emission on Nearby Spiral Galaxies in the IFU Era

open access: yesAdvances in Astronomy, Volume 2013, Issue 1, 2013., 2013
A new generation of wide‐field emission‐line surveys based on integral field units (IFU) is allowing us to obtain spatially resolved information of the gas‐phase emission in nearby late‐type galaxies, based on large samples of HII regions and full two‐dimensional coverage.
Fernando Fabián Rosales-Ortega   +1 more
wiley   +1 more source

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