Results 61 to 70 of about 37,456 (169)
Authentic Leadership—A Concept Analysis
Journal of Advanced Nursing, Volume 81, Issue 4, Page 1775-1793, April 2025.ABSTRACT Aim To report an analysis of the concept of authentic leadership. Design Concept analysis. Data Sources Data sources included core databases: CINAHL, PubMed, Embase, ProQuest, APA PsycINFO, ERIC, ABI/Inform and Tomlinson's Nursing Core Collection (2010).
Mariam Almutairi +4 more
wiley +1 more source
Agency costs of stakeholderism: Evidence from compensation contracting at AT&T
Journal of Applied Corporate Finance, EarlyView.
Stephen Bryan, Robert Nash, Ajay Patel
wiley +1 more source
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The Astrophysical Journal, 2003 23 pages, 3 figures, accepted for publication in ApJ, a new table and several comments ...
openaire +4 more sources
Spectroscopy and 3D imaging of the Crab nebula
, 2004 Spectroscopy of the Crab nebula along different slit directions reveals the 3 dimensional structure of the optical nebula. On the basis of the linear radial expansion result first discovered by Trimble (1968), we make a 3D model of the optical emission ...
Alberto Carraminana +7 more
core +1 more source
PAH and H2emission in the Ring Nebula
Journal of Physics: Conference Series, 2016 This paper presents the Spitzer IRS (Infra Red Spectrograph) detection of mid-infrared polycyclic aromatic hydrocarbon (PAH) emission features and H2 associated with dense knots in the ring of the "oxygen-rich" (C/O~0.6-0.8) planetary nebula (PN) NGC6720 (Ring Nebula). We explored a further three oxygen-rich extended PNe with similar dataset available.
Nick L. J. Cox +8 more
openaire +4 more sources
Fermi Detection of the Pulsar Wind Nebula HESS J1640-465
, 2010 We present observations of HESS J1640-465 with the Fermi-LAT. The source is detected with high confidence as an emitter of high-energy gamma-rays.
Castro, D. +6 more
core +3 more sources
The Ultraviolet Emission Spectra of Planetary Nebulae [PDF]
Symposium - International Astronomical Union, 1968 Calculations show that high-excitation planetaries emit about the same total intensity of collisionally excited radiation in the unobserved ultraviolet part of the spectrum as in the visible. This ultraviolet radiation emanates from a central zone where the electron temperature is high due to absorption of He II Ly-α photons. Intensities of lines which
openaire +2 more sources
A BROADBAND EMISSION MODEL OF MAGNETAR WIND NEBULAE [PDF]
The Astrophysical Journal, 2016 Angular momentum loss by the plasma wind is considered as a universal feature of isolated neutron stars including magnetars. The wind nebulae powered by magnetars allow us to compare the wind properties and the spin-evolution of magnetars with those of rotation-powered pulsars (RPPs).
openaire +4 more sources
Emission-Line Profiles in Planetary Nebulae [PDF]
Symposium - International Astronomical Union, 1968 This research was undertaken with the idea of measuring as accurately as possible the internal-velocity distribution in planetary nebulae, in order to compare the observational measurements with hydrodynamical models of expanding nebulae. Much of the work was done in collaboration with J. S. Miller and D.W. Weedman.
openaire +2 more sources
, 2015 We have monitored the 2014 superoutburst of the WZ Sge-type transient PNV J03093063+2638031 for more than four months, from V=11.0 maximum brightness down to V=18.4 mag, close to quiescence value, by obtaining BVRI photometry and low resolution fluxed ...
Cherini, G. +3 more
core +1 more source