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1

MARINE PALEOENVIRONMENTS OF MIOCENEPLIOCENE FORMATIONS OF NORTH-CENTRAL FALCO N STATE, VENEZUELA  

E-Print Network [OSTI]

MARINE PALEOENVIRONMENTS OF MIOCENE­PLIOCENE FORMATIONS OF NORTH-CENTRAL FALCO´ N STATE, VENEZUELA Venezuela, were used in determinations of the marine paleoenvironments of the Urumaco, Codore, Caujarao, La sequences of Falco´n are compared to other formations of Venezuela and Colombia with similar

Bermingham, Eldredge

2

Breaking news: Biological control agent for Thaumastocoris peregrinus to be released in South Africa  

E-Print Network [OSTI]

milestone in terms of ensuring sustainable plantation forestry in South Africa was safe to release in South Africa as a biological control agent. The release strategy for C. noackae in South Africa must still be finalized. But

3

E-Print Network 3.0 - american kestrel falco Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

and Lincer ... Source: Bortolotti, Gary R. - Department of Biology, University of Saskatchewan Collection: Environmental Sciences and Ecology 8 Journal of Toxicology and...

4

E-Print Network 3.0 - acridine orange Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

orange, grape, parasitoids, host size selection... of acridine orange, a DNA binding dye used to label C. peregrinus eggs. In a choice test, adult parasitoids... was filmed and...

5

E-Print Network 3.0 - affecting eggshell quality Sample Search...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

Captive American kestrels (Falco sparverius) were bred for one... . EMF exposure affected reproductive success of kestrels, increasing fertility, egg size, embryonic Source:...

6

TrekISM Issue 11  

E-Print Network [OSTI]

successful in eradicating this affliction. The following Starho(l)tsnl'l.vebeen perpetrated by one of our newer members I Mike Koenigsberg (P.O.Box 272, Hibbing, MN 55746) * What is the Horta's favorite occupation? ??Hortaculture, naturally. *Wha t is a...'s in diameter (AU=Astronomical unit the distance from E~th t~_the su~) 10=Chief DiFalco l~=wh~n Kirk m~es an entry in the' Captain's Log 12= Kirk 13-a securJ.ty guard 14=a commumcatJ.ons stahon 15-,Kirk, "Thataway" 16=Chief DiFalco 17: McCoy ~8=ma...

1980-01-01T23:59:59.000Z

7

Effects of corticosterone pellets on baseline and stress-induced corticosterone and corticosteroid-binding-globulin  

E-Print Network [OSTI]

Effects of corticosterone pellets on baseline and stress-induced corticosterone and corticosteroid-degradable corticosterone pellets (implanted under the skin) in elevating plasma corticosterone levels. We monitored to handling in Eurasian kestrel Falco tinnunculus and barn owl Tyto alba nestlings. Corticosterone pellets

Alvarez, Nadir

8

Abstract Bird mortality is heavily affected by birds of prey. Under attack, take-off is crucial for survival and  

E-Print Network [OSTI]

Abstract Bird mortality is heavily affected by birds of prey. Under attack, take-off is crucial respond differently depending on the character of the predator's attack and these split-second decisions were studied using a model merlin (Falco columbarius) that attacked feeding blue tits (Parus caeruleus

9

JOURNAL DE PHYSIQUE Colloque C6, suppliment au no 8, Tome 39, aozit 1978, page C6-529 LASER IRRADIATION EFFECTS IN SUPERCONDUCTORS  

E-Print Network [OSTI]

- elded cryostat using a fiber optic bundle which pro- ponse was found to be independent of frequency up IRRADIATION EFFECTS IN SUPERCONDUCTORS C.M. Falco and I.K. schuller' Argonne National kboratory, Argonne mince et d'une boucle supraconductricebim6tallique sous irradiation d'une lumisre laser. Nous trouvons

Boyer, Edmond

10

The radial velocity profile of the filament galaxies in the vicinity of the Virgo cluster as a test of gravity  

E-Print Network [OSTI]

The radial velocities of the galaxies in the vicinity of a massive cluster shows deviation from the pure Hubble flow due to their gravitational interaction with the cluster. According to a recent study of Falco et al. with a high-resolution N-body simulation based on General Relativity (GR), the radial velocity profile of the galaxies located at distances larger than three times the virial radius of a neighbour cluster has a universal shape and could be reconstructed from direct observables provided that the galaxies are distributed along one dimensional filament. Analyzing the narrow filamentary structure identified by Kim et al. in the vicinity of the Virgo cluster from the NASA-Sloan-Atlas catalog, we reconstruct the radial velocity profile of the Virgo filament galaxies and compare it with the universal formula derived by Falco et al. It is found that unless the virial mass of the Virgo cluster exceeds $10^{15}\\,h^{-1}M_{\\odot}$ the universal formula fails to describe the reconstructed radial velocity pro...

Lee, Jounghun; Rey, Soo-Chang

2015-01-01T23:59:59.000Z

11

Quantum-corrected drift-diffusion models: Solution fixed point map and finite element approximation  

SciTech Connect (OSTI)

This article deals with the analysis of the functional iteration, denoted Generalized Gummel Map (GGM), proposed in [C. de Falco, A.L. Lacaita, E. Gatti, R. Sacco, Quantum-Corrected Drift-Diffusion Models for Transport in Semiconductor Devices, J. Comp. Phys. 204 (2) (2005) 533-561] for the decoupled solution of the Quantum Drift-Diffusion (QDD) model. The solution of the problem is characterized as being a fixed point of the GGM, which permits the establishment of a close link between the theoretical existence analysis and the implementation of a numerical tool, which was lacking in previous non-constructive proofs [N.B. Abdallah, A. Unterreiter, On the stationary quantum drift-diffusion model, Z. Angew. Math. Phys. 49 (1998) 251-275, R. Pinnau, A. Unterreiter, The stationary current-voltage characteristics of the quantum drift-diffusion model, SIAM J. Numer. Anal. 37 (1) (1999) 211-245]. The finite element approximation of the GGM is illustrated, and the main properties of the numerical fixed point map (discrete maximum principle and order of convergence) are discussed. Numerical results on realistic nanoscale devices are included to support the theoretical conclusions.

Falco, Carlo de [School of Mathematical Sciences, Dublin City University, Glasnevin, Dublin 9 (Ireland); Jerome, Joseph W. [Department of Mathematics, Northwestern University, 2033 Sheridan Road, Evanston, IL 60208-2730 (United States); Sacco, Riccardo [Dipartimento di Matematica 'F.Brioschi', Politecnico di Milano, via Bonardi 9, 20133 Milano (Italy)], E-mail: riccardo.sacco@polimi.it

2009-03-20T23:59:59.000Z

12

Emission-Line Galaxy Surveys as Probes of the Spatial Distribution of Dwarf Galaxies. I. The University of Michigan Survey  

E-Print Network [OSTI]

Objective-prism surveys which select galaxies on the basis of line-emission are extremely effective at detecting low-luminosity galaxies and constitute some of the deepest available samples of dwarfs. In this study, we confirm that emission-line galaxies (ELGs) in the University of Michigan (UM) objective-prism survey (MacAlpine et al. 1977-1981) are reliable tracers of large-scale structure, and utilize the depth of the samples to examine the spatial distribution of low-luminosity (M$_{B} > $ -18.0) dwarfs relative to higher luminosity giant galaxies (M$_{B} \\leq$ -18.0) in the Updated Zwicky Catalogue (Falco et al. 1999). New spectroscopic data are presented for 26 UM survey objects. We analyze the relative clustering properties of the overall starbursting ELG and normal galaxy populations, using nearest neighbor and correlation function statistics. This allows us to determine whether the activity in ELGs is primarily caused by gravitational interactions. We conclude that galaxy-galaxy encounters are not the sole cause of activity in ELGs since ELGs tend to be more isolated and are more often found in the voids when compared to their normal galaxy counterparts. Furthermore, statistical analyses performed on low-luminosity dwarf ELGs show that the dwarfs are less clustered when compared to their non-active giant neighbors. The UM dwarf samples have greater percentages of nearest neighbor separations at large values and lower correlation function amplitudes relative to the UZC giant galaxy samples. These results are consistent with the expectations of galaxy biasing.

Janice C. Lee; John J. Salzer; Jessica Rosenberg; Daniel Law

2000-01-21T23:59:59.000Z