Zobrazeno 1 - 10
of 32
pro vyhledávání: '"B. L. de Vries"'
Publikováno v:
Icarus, 307, 400-416. Academic Press Inc.
Meteorites contain minerals from Solar System asteroids with differentproperties (like size, presence of water, core formation). We providenew mid-IR transmission spectra of powdered meteorites to obtaintemplates of how mid-IR spectra of asteroidal d
Autor:
Ulrich Wahl, E. David-Bosne, L. M. C. Pereira, L. M. Amorim, André Vantomme, B. L. de Vries, M.R. da Silva, J. G. Correia, A. R. G. Costa
Publikováno v:
Journal of Applied Physics
The lattice location of ion implanted radioactive 24Na (t1/2=14.96 h) in GaN and AlN was determined using the emission channeling technique at the ISOLDE/CERN facility. In the room temperature as-implanted state in both GaN and AlN, the majority of t
Publikováno v:
EAS Publications Series. :65-70
The superwind is believed to be the tool with which stars with an intermediate main-sequence mass between 5 and 8 Me shed most of their stellar mantle to evolve from the asymptotic giant branch (AGB) into the post-AGB and planetary-nebulae stages. Fo
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms. 267:1340-1344
A GaN thin film was implanted with 5 × 1014 cm−2 of 60 keV stable 166Er, followed by the implantation of 2 × 1013 cm−2 radioactive 167Tm (t1/2 = 9.3 d) and an annealing sequence up to 900 °C. The emission channeling (EC) technique was applied
Autor:
Nick L. J. Cox, B. L. de Vries, Leen Decin, Michiel Min, L. B. F. M. Waters, A. de Koter, Theo Khouri, Robin Lombaert
Publikováno v:
Astronomy & Astrophysics, 577:A114. EDP Sciences
Low- and intermediate-mass stars go through a period of intense mass-loss at the end of their lives in a phase known as the asymptotic giant branch (AGB). During the AGB a significant fraction of their initial mass is expelled in a stellar wind. This
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e3e308bfef62573e3f030ad4e1305c2b
http://arxiv.org/abs/1503.04765
http://arxiv.org/abs/1503.04765
Autor:
L.B.F.M. Waters, Michiel Min, K. M. Maaskant, J. A. D. L. Blommaert, B. L. de Vries, Robin Lombaert
Publikováno v:
Astronomy & Astrophysics, 576, A98
Astronomy & Astrophysics, 576:A98. EDP Sciences
Astronomy & Astrophysics, 576:A98. EDP Sciences
We study the grain properties and location of the forsterite crystals in the circumstellar environment of the pre-planetary nebula (PPN) IRAS 17150-3224 in order to learn more about the as yet poorly understood evolutionary phase prior to the PPN. We
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0cb71e36ebf12ab7854d298a6f7ff083
https://dare.uva.nl/personal/pure/en/publications/micronsized-forsterite-grains-in-the-preplanetary-nebula-of-iras-171503224-searching-for-clues-to-the-mysterious-evolution-of-massive-agb-stars(19348c67-fa85-44de-a8ab-0303d3f61694).html
https://dare.uva.nl/personal/pure/en/publications/micronsized-forsterite-grains-in-the-preplanetary-nebula-of-iras-171503224-searching-for-clues-to-the-mysterious-evolution-of-massive-agb-stars(19348c67-fa85-44de-a8ab-0303d3f61694).html
Autor:
Reiner Vianden, Katharina Lorenz, Ulrich Wahl, J. G. Correia, André Vantomme, Teresa Monteiro, B. L. de Vries, Eduardo Alves
Publikováno v:
Repositório Científico de Acesso Aberto de Portugal
Repositório Científico de Acesso Aberto de Portugal (RCAAP)
instacron:RCAAP
Repositório Científico de Acesso Aberto de Portugal (RCAAP)
instacron:RCAAP
This paper reviews the current knowledge on rare earths (REs) implanted into GaN with a special focus on their lattice location and on the optical activation by means of thermal annealing. While emission channeling experiments have given information
Publikováno v:
Materials Science and Engineering: B. 105:106-110
The lattice site location of excited states of 149 Eu was studied by means of the emission channeling technique. The 60 keV implantation of 149 Tb into a GaN thin film was performed at room temperature up to a dose of 2.0×1013 cm−2. This radioacti
Publikováno v:
Journal of Physics: Condensed Matter. 14:3275-3283
The energy-versus-volume curve of the spin-density wave (SDW) in body-centred-cubic Cr is calculated with the density functional theory/full-potential linearized augmented plane wave (DFT/FLAPW) method using the generalized gradient approximation (GG
Autor:
J. A. D. L. Blommaert, Walter Kieran Gear, Wayne S. Holland, B. L. de Vries, G. Olofsson, B. Sibthorpe, Brenda C. Matthews, Sam Lawler, Bart Vandenbussche, Grant M. Kennedy, Ana M. Heras, Mark Booth, Carsten Dominik, Rob Ivison, Mikko Tuomi, Malcolm Fridlund, David J. Wilner, J. Di Francesco, Jane Greaves
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 444, 3, pp. 2665-2675
Monthly Notices of the Royal Astronomical Society, 444, 2665-2675
Monthly Notices of the Royal Astronomical Society, 444(3), 2665-2675. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 444, 2665-2675
Monthly Notices of the Royal Astronomical Society, 444(3), 2665-2675. Oxford University Press
$\tau$ Ceti is a nearby, mature G-type star very similar to our Sun, with a massive Kuiper Belt analogue (Greaves et al. 2004) and possible multiplanet system (Tuomi et al. 2013) that has been compared to our Solar System. We present Herschel Space O
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f0659e142a8ec05cd5c5cc900fa47407
https://hdl.handle.net/10023/5835
https://hdl.handle.net/10023/5835