Zobrazeno 1 - 10
of 30
pro vyhledávání: '"G. C. Murphy"'
Autor:
Niall Cullinane, G. C. Murphy
Publikováno v:
Murphy, G & Cullinane, N 2021, ' Performance management technologies and trade union responses: A case study from banking ', New Technology, Work and Employment . https://doi.org/10.1111/ntwe.12207
Literature in the Performance Management (PM) field champions a shift to more continual forms of worker assessment. Advances in data analytic technologies are claimed to support such developments. However, critical literature finds that PM technologi
Autor:
G. C. Murphy, Niall Cullinane
Publikováno v:
Cullinane, N & Murphy, G 2021, ' Bargaining, representation and organising in the Pandemic: Experience from the Financial Services Union ', International Union Rights: Journal of the International Centre for Trade Union Rights, vol. 28, no. 2, pp. 20-21 . https://doi.org/10.14213/inteuniorigh.28.2.0020
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4c78422a6f77b66f3e156e37163090cc
https://pure.qub.ac.uk/en/publications/95abeea8-761d-4422-8283-6c54c3231d44
https://pure.qub.ac.uk/en/publications/95abeea8-761d-4422-8283-6c54c3231d44
Autor:
G. Pelletier, B. Lembege, A. Stockem Novo, Lorenzo Sironi, G. Morlino, Brian Reville, Mario Riquelme, M. E. Dieckman, L. O. C. Drury, Martin Lemoine, A. M. Bykov, A. Marcowith, G. C. Murphy, Illya Plotnikov, Antoine Bret
Publikováno v:
Reports on Progress in Physics
Reports on Progress in Physics, IOP Publishing, 2016, 79 (4), pp.046901. ⟨10.1088/0034-4885/79/4/046901⟩
Reports on Progress in Physics, 2016, 79 (4), pp.046901. ⟨10.1088/0034-4885/79/4/046901⟩
Reports on Progress in Physics, IOP Publishing, 2016, 79 (4), pp.046901. 〈10.1088/0034-4885/79/4/046901〉
Marcowith, A, Bret, A, Bykov, A, Dieckmann, M, Drury, L, Lembege, B, Lemoine, M, Morlino, G, Murphy, G, Pelletier, G, Plotnikov, I, Reville, B, Riquelme, M, Sironi, L & Stockem Novo, A 2016, ' The microphysics of collisionless shock waves ', Reports on Progress in Physics, vol. 79, no. 4, 046901 . https://doi.org/10.1088/0034-4885/79/4/046901
Reports on Progress in Physics, IOP Publishing, 2016, 79 (4), pp.046901. ⟨10.1088/0034-4885/79/4/046901⟩
Reports on Progress in Physics, 2016, 79 (4), pp.046901. ⟨10.1088/0034-4885/79/4/046901⟩
Reports on Progress in Physics, IOP Publishing, 2016, 79 (4), pp.046901. 〈10.1088/0034-4885/79/4/046901〉
Marcowith, A, Bret, A, Bykov, A, Dieckmann, M, Drury, L, Lembege, B, Lemoine, M, Morlino, G, Murphy, G, Pelletier, G, Plotnikov, I, Reville, B, Riquelme, M, Sironi, L & Stockem Novo, A 2016, ' The microphysics of collisionless shock waves ', Reports on Progress in Physics, vol. 79, no. 4, 046901 . https://doi.org/10.1088/0034-4885/79/4/046901
Collisionless shocks, that is shocks mediated by electromagnetic processes, are customary in space physics and in astrophysics. They are to be found in a great variety of objects and environments: magnetospheric and heliospheric shocks, supernova rem
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e8292d85f7951240b39f322b66987f70
https://hal-insu.archives-ouvertes.fr/insu-01292937
https://hal-insu.archives-ouvertes.fr/insu-01292937
Publikováno v:
International Journal of Modern Physics: Conference Series. :376-379
Gamma ray bursts (GRBs) are thought to originate from highly relativistic jets. The fireball model predicts internal shocks in the jets, causing magnetic field to be amplified and particles to be accelerated. We model the effects of an asymmetric den
Publikováno v:
International Journal of Modern Physics D. 19:707-713
A gamma-ray burst (GRB) is triggered by a stellar implosion and the subsequent ejection of an ultrarelativistic jet. The prompt emissions are attributed to mildly relativistic collisions of plasma clouds within this jet. The resulting internal shocks
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2005, 432, pp.575. ⟨10.1051/0004-6361:20041791⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2005, 432, pp.575. ⟨10.1051/0004-6361:20041791⟩
We present a large-scale study of the IC1396 region using new deep NIR and optical images, complemented by 2MASS data. For ten globules in IC1396 we determine (H-K, J-H) colour-colour diagrams and identify the young stellar population. Five of these
Publikováno v:
Astrophysics and Space Science. 293:263-269
It is commonly accepted that stars form in molecular clouds by the gravitational collapse of dense gas. However, it is precisely not the infalling but the outflowing material that is primarily observed. Outflow motions prevail around both low and hig
Autor:
G. C. Murphy, Martin E. Pessah
Publikováno v:
Murphy, G & Pessah, M E 2015, ' On the Anisotropic Nature of MRI-driven Turbulence in Astrophysical Disks ', Astrophysical Journal, vol. 802, no. 2, 139 . https://doi.org/10.1088/0004-637X/802/2/139
The magnetorotational instability is thought to play an important role in enabling accretion in sufficiently ionized astrophysical disks. The rate at which MRI-driven turbulence transports angular momentum is related to both the strength of the ampli
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5d7e0a0f268a6a78ff8b604df918bc0b
The energetic electromagnetic eruptions observed during the prompt phase of gamma-ray bursts are attributed to synchrotron emissions. The internal shocks moving through the ultrarelativistic jet, which is ejected by an imploding supermassive star, ar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::906f6cfcdbb4eb07497579c7129c775a
http://arxiv.org/abs/1011.4406
http://arxiv.org/abs/1011.4406
The prompt emissions of gamma-ray bursts are seeded by radiating ultrarelativistic electrons. Internal shocks propagating through a jet launched by a stellar implosion, are expected to amplify the magnetic field & accelerate electrons. We explore the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0c835d5a193f690e3bfcec1288963277
http://arxiv.org/abs/1010.1146
http://arxiv.org/abs/1010.1146