Zobrazeno 1 - 10
of 486
pro vyhledávání: '"J van Marle"'
Publikováno v:
Journal of Lipid Research, Vol 30, Iss 1, Pp 51-58 (1989)
Human bile contains a factor with cholesterol nucleation-promoting activity that binds to concanavalin A-Sepharose. In this study we have investigated the effect of this activity on the dynamics of lipid solubilization in supersaturated model bile. A
Externí odkaz:
https://doaj.org/article/88fc6b1d7b454083bea3590d6548d093
Autor:
A A Chrimes, B P Gompertz, D A Kann, A J van Marle, J J Eldridge, P J Groot, T Laskar, A J Levan, M Nicholl, E R Stanway, K Wiersema
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 515, 2591-2611
Monthly Notices of the Royal Astronomical Society, 515, 2, pp. 2591-2611
Monthly Notices of the Royal Astronomical Society, 515, 2, pp. 2591-2611
The temporal and spectral evolution of gamma-ray burst (GRB) afterglows can be used to infer the density and density profile of the medium through which the shock is propagating. In long-duration (core-collapse) GRBs, the circumstellar medium (CSM) i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8849f761a0f58ef2756385955694a60e
https://doi.org/10.1093/mnras/stac1796
https://doi.org/10.1093/mnras/stac1796
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 482(4), 5052-5077. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 482(4), 5052-5077. Oxford University Press
The material lost through stellar winds of Asymptotic Giant Branch (AGB) stars is one of the main contributors to the chemical enrichment of galaxies. The general hypothesis of the mass loss mechanism of AGB winds is a combination of stellar pulsatio
Publikováno v:
Phys.Plasmas
Phys.Plasmas, 2021, 28 (8), pp.080601. ⟨10.1063/5.0013662⟩
Physics of Plasmas
Physics of Plasmas, 2021, 28 (8), pp.080601. ⟨10.1063/5.0013662⟩
Phys.Plasmas, 2021, 28 (8), pp.080601. ⟨10.1063/5.0013662⟩
Physics of Plasmas
Physics of Plasmas, 2021, 28 (8), pp.080601. ⟨10.1063/5.0013662⟩
International audience; Energetic non-thermal particles, or cosmic rays, are a major component of astrophysical plasmas next to magnetic fields, radiation, and thermal gas. Cosmic rays are usually sub-dominant in density but carry as much pressure as
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5572d4557d8114f15562dac4fb47862a
https://hal.archives-ouvertes.fr/hal-03335769
https://hal.archives-ouvertes.fr/hal-03335769
A 70-year-old man was admitted to our hospital for a penile circumcision due to phimosis using continuous dose spinal anaesthesia. On postoperative day 10 he came to the emergency department with a superficial abscess localised at the injection site
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e18ea93872aed7c23d91185985af7848
https://europepmc.org/articles/PMC5847936/
https://europepmc.org/articles/PMC5847936/
Publikováno v:
Plasma Phys.Control.Fusion
44th European Physical Society Conference on Plasma Physics
44th European Physical Society Conference on Plasma Physics, Jun 2017, Belfast, Ireland. pp.014017, ⟨10.1088/1361-6587/aa8482⟩
44th European Physical Society Conference on Plasma Physics
44th European Physical Society Conference on Plasma Physics, Jun 2017, Belfast, Ireland. pp.014017, ⟨10.1088/1361-6587/aa8482⟩
International audience; We present simulations of magnetized astrophysical shocks taking into account the interplay between the thermal plasma of the shock and supra-thermal particles. Such interaction is depicted by combining a grid-based magneto-hy
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2b6666e328035a24c77d9bc660d0397f
https://hal.archives-ouvertes.fr/hal-02101712
https://hal.archives-ouvertes.fr/hal-02101712
The influence of a variable mass loss rate on the dust and gas dynamics in the bow-shock ofα-Orionis
Autor:
L. Decin, A. J. van Marle
Publikováno v:
EAS Publications Series. 60:235-241
We present hydrodynamical simulations of the interaction between the stellar wind of α -Orionis and the interstellar gas. In particular we focus our efforts on reproducing the multiple arc structure of the bow-shock that was observed with Herschel.
Publikováno v:
EAS Publications Series. 60:227-234
Context. The interaction between stellar winds and the interstellar medium (ISM) can create complex bow shocks. The photometers on board the Herschel Space Observatory are ideally suited to studying the morphologies of these bow shocks. Aims. We aim
Publikováno v:
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2016, 459 (2), pp.1146-1158. ⟨10.1093/mnras/stw651⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2016, 459 (2), pp.1146-1158. ⟨10.1093/mnras/stw651⟩
Monthly Notices of the Royal Astronomical Society, 2016, 459 (2), pp.1146-1158. ⟨10.1093/mnras/stw651⟩
Mon.Not.Roy.Astron.Soc., 2016, 459 (2), pp.1146-1158. 〈10.1093/mnras/stw651〉
Mon.Not.Roy.Astron.Soc., 2016, 459 (2), pp.1146-1158. ⟨10.1093/mnras/stw651⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2016, 459 (2), pp.1146-1158. ⟨10.1093/mnras/stw651⟩
Monthly Notices of the Royal Astronomical Society, 2016, 459 (2), pp.1146-1158. ⟨10.1093/mnras/stw651⟩
Mon.Not.Roy.Astron.Soc., 2016, 459 (2), pp.1146-1158. 〈10.1093/mnras/stw651〉
Massive stars that have been ejected from their parent cluster and supersonically sailing away through the interstellar medium (ISM) are classified as exiled. They generate circumstellar bow shock nebulae that can be observed. We present two-dimensio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::33b670238d7223be499908220e4c2ec7
https://hal.archives-ouvertes.fr/hal-01582432
https://hal.archives-ouvertes.fr/hal-01582432
Publikováno v:
Biochemistry and Cell Biology. 90:378-388
Bovine lactoferrin harbors 2 antimicrobial sequences (LFcin and LFampin), situated in close proximity in the N1-domain. To mimic their semi parallel configuration we have synthesized a chimeric peptide (LFchimera) in which these sequences are linked