User profiles for Simon Albrecht
![]() | Simon AlbrechtAarhus University, Denmark Verified email at phys.au.dk Cited by 12011 |
Key questions regarding work engagement
This article discusses the concept of work engagement and summarizes research on its
most important antecedents. The authors formulate 10 key questions and shape a research …
most important antecedents. The authors formulate 10 key questions and shape a research …
Work engagement: current trends
AB Bakker, S Albrecht - Career development international, 2018 - emerald.com
Over the past two decades, the number of studies on work engagement has increased
rapidly. Work engagement refers to a positive, affective-motivational state of high energy …
rapidly. Work engagement refers to a positive, affective-motivational state of high energy …
Employee engagement, human resource management practices and competitive advantage: An integrated approach
Purpose – The purpose of this paper is to argue in support of a model that shows how four
key HRM practices focused on engagement influence organizational climate, job demands …
key HRM practices focused on engagement influence organizational climate, job demands …
Stellar obliquities in exoplanetary systems
SH Albrecht, RI Dawson, JN Winn - Publications of the …, 2022 - iopscience.iop.org
The rotation of a star and the revolutions of its planets are not necessarily aligned. This article
reviews the measurement techniques, key findings, and theoretical interpretations related …
reviews the measurement techniques, key findings, and theoretical interpretations related …
Obliquities of hot Jupiter host stars: Evidence for tidal interactions and primordial misalignments
We provide evidence that the obliquities of stars with close-in giant planets were initially
nearly random, and that the low obliquities that are often observed are a consequence of star–…
nearly random, and that the low obliquities that are often observed are a consequence of star–…
Low stellar obliquities in compact multiplanet systems
We measure the sky-projected stellar obliquities (λ) in the multiple-transiting planetary systems
KOI-94 and Kepler-25, using the Rossiter–McLaughlin effect. In both cases, the host stars …
KOI-94 and Kepler-25, using the Rossiter–McLaughlin effect. In both cases, the host stars …
The orbital motion, absolute mass and high-altitude winds of exoplanet HD 209458b
For extrasolar planets discovered using the radial velocity method 1 , the spectral characterization
of the host star leads to a mass estimate of the star and subsequently of the orbiting …
of the host star leads to a mass estimate of the star and subsequently of the orbiting …
Hot stars with hot Jupiters have high obliquities
JN Winn, D Fabrycky, S Albrecht… - The Astrophysical …, 2010 - iopscience.iop.org
We show that stars with transiting planets for which the stellar obliquity is large are
preferentially hot (T eff> 6250 K). This could explain why small obliquities were observed in the …
preferentially hot (T eff> 6250 K). This could explain why small obliquities were observed in the …
Work engagement: Further reflections on the state of play
In this article we further reflect on the “state of play” of work engagement. We consider, clarify,
and respond to issues and themes raised by eight preeminent work engagement …
and respond to issues and themes raised by eight preeminent work engagement …
Misaligned spin and orbital axes cause the anomalous precession of DI Herculis
The orbits of binary stars precess as a result of general relativistic effects, forces arising from
the asphericity of the stars, and forces from any additional stars or planets in the system. For …
the asphericity of the stars, and forces from any additional stars or planets in the system. For …