Zobrazeno 1 - 10
of 18
pro vyhledávání: '"Zeinab Khorrami"'
Publikováno v:
Journal of Soils and Sediments. 21:545-560
This paper reports the development of a non-coupled algorithm and its application in a real case study. The main objective was to provide 2D/3D, long-term simulation of dam reservoir sedimentation by removing the part of calculations which did not si
Publikováno v:
International Journal of Sediment Research. 34:279-294
This paper investigates the validity of a quasi-steady approximation for sediment transport and presents a new algorithm based on this concept. The developed non-coupled algorithm interacts among hydrodynamic, sediment, and morphology modules which a
Publikováno v:
Applied Mathematical Modelling. 67:378-398
This paper aims at developing a multi-block sigma-coordinate to simulate morphological evolutions. The developed multi-block sigma-coordinate can represent a steep slope topography smoothly with different numbers of horizontal layers, without produci
Autor:
Anne S. M. Buckner, Zeinab Khorrami, Marta González, Stuart L. Lumsden, Paul Clark, Estelle Moraux
[Context.] Gaia is limited in the optical down to G~21 mag so it is essential to understand the biases introduced by a magnitude-limited sample on spatial distribution studies. [Aims.] We ascertain how sample incompleteness in Gaia observations of yo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::84fcb0d96cd0fffe8cc5a655a2198e82
Autor:
Marta González, Anne S. M. Buckner, Maud Langlois, Paul C. Clark, Estelle Moraux, Stuart Lumsden, F. Vakili, Jan Palouš, Paul A. Crowther, Richard Wünsch, Zeinab Khorrami
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2021, 503, pp.292-311. ⟨10.1093/mnras/stab388⟩
Monthly Notices of the Royal Astronomical Society, 2021, 503, pp.292-311. ⟨10.1093/mnras/stab388⟩
We present the sharpest and deepest near infrared photometric analysis of the core of R136, a newly formed massive star cluster at the centre of the 30 Doradus star forming region in the Large Magellanic Cloud. We used the extreme adaptive optics of
Autor:
Rene D. Oudmaijer, Jose Manuel Blanco, Paul C. Clark, Isabelle Joncour, Jose Maria Herrera-Fernandez, Stuart Lumsden, Estelle Moraux, Zeinab Khorrami, Pouria Khalaj, Luis Valero-Martin, Anne S. M. Buckner, Frédérique Motte, Ignacio de la Calle
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2019, ⟨10.1093/mnras/stz490⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2019, ⟨10.1093/mnras/stz490⟩
We introduce our new code MYOSOTIS (Make Your Own Synthetic ObservaTIonS) which is designed to produce synthetic observations from simulated clusters. The code can synthesise observations from both ground- and spaced-based observatories, for a range
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::12fbb7dab4947ebe14db74a13e0ff38c
https://hal.archives-ouvertes.fr/hal-02416600
https://hal.archives-ouvertes.fr/hal-02416600
Autor:
Estelle Moraux, Rene D. Oudmaijer, Jose Manuel Blanco, Paul C. Clark, Pouria Khalaj, Stuart Lumsden, Isabelle Joncour, Jose Maria Herrera-Fernandez, Zeinab Khorrami, Luis Valero-Martin, Jesus Salgado, Ignacio de la Calle, Anne S. M. Buckner, Frédérique Motte
Aims. To present the new novel statistical clustering tool 'INDICATE' which assesses and quantifies the degree of spatial clustering of each object in a dataset, discuss its applications as a tracer of morphological stellar features in star forming r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8de0c8308c46dd086000160c7db2d917
http://arxiv.org/abs/1901.02371
http://arxiv.org/abs/1901.02371
Publikováno v:
EAS Publications Series. :331-335
As most stars are born in a clustered mode, young massive star clusters are the best places to find and study the formation and evolution of massive stars. R136 is one of the most massive nearby clusters in the LMC. It contains at least 72 known O an
Publikováno v:
International Journal of Sediment Research. 34:399
Autor:
D. Schertl, A. Domiciano de Souza, T. Lanz, P Berio, G. Niccolini, F. Thévenin, Josef Hron, Karl-Heinz Hofmann, P. Bendjoya, Florentin Millour, Romain Petrov, A. Soulain, Ph. Stee, Zeinab Khorrami, N. Nardetto, A Meilland, Bruno Lopez, Claudia Paladini, F. Vakili, Alexis Matter, Andrea Chiavassa, P. Cruzalebes, Gerd Weigelt
Publikováno v:
SPIE
SPIE, Jun 2016, Edimbourgh, France
HAL
SPIE, Jun 2016, Edimbourgh, France
HAL
MATISSE represents a great opportunity to image the environment around massive and evolved stars. This will allow one to put constraints on the circumstellar structure, on the mass ejection of dust and its reorganization , and on the dust-nature and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2d6c4976cfb59b6ec269777145c85ea4