Results 71 to 80 of about 150,777 (255)

Efeito da luz e da quebra de dormência na germinação de sementes de espécies de plantas daninhas Effect of light and dormancy break on weed species seed germination

open access: yesPlanta Daninha, 2007
Objetivou-se com este trabalho verificar a quebra de dormência, utilizando ácido sulfúrico (H2SO4) e escarificação mecânica, e o efeito da luz na germinação das espécies Euphorbia heterophylla, Ipomoea nil, Sida glaziovii e Brachiaria plantaginea.
F.L. Salvador   +4 more
doaj   +1 more source

Thermal Energy and Luminosity Characterization of an Advanced Ignition System Using a Non-Intrusive Methodology in an Optically Accessible Calorimeter

open access: yesEnergies, 2023
To restrain the environmental impact of modern SI engines, igniters must guarantee stable combustions with low cycle-to-cycle variability in extreme operating conditions (high EGR, ultra-lean), via high energy release in the combustion chamber.
Roberto Martinelli   +5 more
doaj   +1 more source

Letter: Note on the Luminosity Distance [PDF]

open access: yesGeneral Relativity and Gravitation, 2004
We re-derive a formula relating the areal and luminosity distances, entirely in the framework of the classical Maxwell theory, assuming a geometric-optics type condition.
Grzegorz Wyleżek   +2 more
openaire   +4 more sources

TOWARD THE STANDARD POPULATION SYNTHESIS MODEL OF THE X-RAY BACKGROUND: EVOLUTION OF X-RAY LUMINOSITY AND ABSORPTION FUNCTIONS OF ACTIVE GALACTIC NUCLEI INCLUDING COMPTON-THICK POPULATIONS [PDF]

open access: yes, 2014
We present the most up to date X-ray luminosity function (XLF) and absorption function of active galactic nuclei (AGNs) over the redshift range from 0 to 5, utilizing the largest, highly complete sample ever available obtained from surveys performed with
Y. Ueda   +4 more
semanticscholar   +1 more source

The bolometric luminosities of stars [PDF]

open access: yesSymposium - International Astronomical Union, 1997
The total energy emitted by a star is one of its basic parameters. It is also one of the most difficult to determine, requiring space-based as well as ground-based measurements of the absolute flux from stars. We review the current status of these observations in the ultraviolet, visible, and near infrared, and estimate the uncertainties of the ...
Jeffrey W. Percival, Robert Bless
openaire   +3 more sources

THE EVOLUTION OF THE GALAXY REST-FRAME ULTRAVIOLET LUMINOSITY FUNCTION OVER THE FIRST TWO BILLION YEARS [PDF]

open access: yes, 2014
We present a robust measurement and analysis of the rest-frame ultraviolet (UV) luminosity functions at z = 4–8. We use deep Hubble Space Telescope imaging over the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey/GOODS fields, the Hubble ...
S. Finkelstein   +28 more
semanticscholar   +1 more source

Luminosity to the Eddington luminosity ratio in AGN

open access: yes, 1996
LaTex file, uses epsfig, 4 pages, 5 Postscript figures, contribution to 2nd INTEGRAL Workshop, "The Transparent Universe", St.
Czerny, B., Witt, H. J., Zycki, P. T.
openaire   +2 more sources

The cepheid luminosity scale [PDF]

open access: yesSpace Science Reviews, 1980
The distances of clusters containing classical Cepheids are central to the calibration of the period-luminosity relation. As a step in improving the reliability of the calibration, uvbys photometry was obtained for B stars in eight of these clusters. These data were then used to determine the distances of the clusters and, thus, the absolute magnitudes
openaire   +4 more sources

A remarkably flat relationship between the average star formation rate and AGN luminosity for distant X-ray AGN. [PDF]

open access: yes, 2015
In this study, we investigate the relationship between the star formation rate (SFR) and AGN luminosity (LAGNLAGN) for ∼2000 X-ray detected AGN.
F. Stanley   +8 more
semanticscholar   +1 more source

THE GALAXY UV LUMINOSITY FUNCTION BEFORE THE EPOCH OF REIONIZATION [PDF]

open access: yesProceedings of the International Astronomical Union, 2015
We present a model for the evolution of the galaxy ultraviolet (UV) luminosity function (LF) across cosmic time where star formation is linked to the assembly of dark matter halos under the assumption of a mass-dependent, but redshift-independent ...
C. Mason, M. Trenti, T. Treu
semanticscholar   +1 more source

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