Results 41 to 50 of about 2,347,766 (295)

The HI content of extremely metal-deficient blue compact dwarf galaxies [PDF]

open access: yes, 2016
We have obtained new HI observations with the 100m Green Bank Telescope (GBT) for a sample of 29 extremely metal-deficient star-forming Blue Compact Dwarf (BCD) galaxies, selected from the Sloan Digital Sky Survey spectral data base to be extremely metal-
Goehring, K. M.   +4 more
core   +2 more sources

The Mass-Richness Relation of MaxBCG Clusters from Quasar Lensing Magnification using Variability

open access: yes, 2012
Accurate measurement of galaxy cluster masses is an essential component not only in studies of cluster physics, but also for probes of cosmology. However, different mass measurement techniques frequently yield discrepant results.
Baltay, Charles   +5 more
core   +1 more source

Kinematic deprojection and mass inversion of spherical systems of known velocity anisotropy [PDF]

open access: yes, 2009
Traditionally, the mass / velocity anisotropy degeneracy (MAD) inherent in the spherical, stationary, non-streaming Jeans equation has been handled by assuming a mass profile and fitting models to the observed kinematical data.
Alard   +58 more
core   +2 more sources

Does Conversion to Organic Farming Impact Vineyards Yield? A Diachronic Study in Southeastern France

open access: yesAgronomy, 2020
Given the need to reduce pesticide use and rising consumer demand for healthy food, organic vineyard areas have increased since 2000. Converting to organic farming requires numerous changes in pest and disease management, fertilization and weeding ...
Anne Merot, Nathalie Smits
doaj   +1 more source

The Double-Lined Spectroscopic Binary Haro 1-14c

open access: yes, 2004
We report detection of the low-mass secondary in the spectroscopic binary Haro 1-14c in the Ophiuchus star forming region. The secondary/primary mass ratio is $0.310\pm 0.014$.
Baraffe I., L. Prato, M. Simon
core   +1 more source

Chemical Yields From Low-and Intermediate-Mass Stars [PDF]

open access: yes, 2000
We present new sets of chemical yields from low- and intermediate-mass stars with 0.8 Msun <= M <= Mup ~ 5 Msun, and three choices of the metallicity, Z=0.02, Z=0.008, and Z=0.004 (Marigo 2000, in preparation). These are then compared with the yields calculated by other authors on the basis of different model prescriptions, and basic ...
openaire   +3 more sources

Self-interfering wavepackets [PDF]

open access: yes, 2015
We study the propagation of non-interacting polariton wavepackets. We show how two qualitatively different concepts of mass that arise from the peculiar polariton dispersion lead to a new type of particle-like object from non-interacting fields---much ...
Colas, David, Laussy, Fabrice
core   +2 more sources

European Standard Clinical Practice Guideline and EXPeRT Recommendations for the Diagnosis and Management of Gastroenteropancreatic Neuroendocrine Neoplasms in Children and Adolescents

open access: yesPediatric Blood &Cancer, EarlyView.
ABSTRACT Pediatric gastroenteropancreatic neuroendocrine neoplasms (GEP‐NENs) are extremely rare and clinically heterogeneous. Management has largely been extrapolated from adult practice. This European Standard Clinical Practice Guideline (ESCP), developed by the EXPeRT network in collaboration with adult NEN experts, provides (adult) evidence ...
Michaela Kuhlen   +23 more
wiley   +1 more source

Effects of torrefaction on energy properties of Eucalyptus grandis wood [PDF]

open access: yes, 2009
Torrefaction is a thermal treatment that promotes homogenization and improvement of energy properties of biomass. This study aims to evaluate the effects of torrefaction on the main energy properties of Eucalyptus grandis wood.
Oliveira Rodrigues, Thiago   +1 more
core  

J/psi production in a gluon plasma produced in Au-Au collisions at the Relativistic Heavy Ion Collider

open access: yes, 2003
Centrality dependence of J/psi production in Au-Au collisions at 200 GeV nucleon-nucleon center of mass energy is studied using the Glauber model plus the kinetic formation model.
Abreu   +69 more
core   +1 more source

Home - About - Disclaimer - Privacy