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pro vyhledávání: '"Lundqvist A"'
Autor:
Abdenbi, El Azri1 a.elazri@uhp.ac.ma, Ahmed, Nafidi1 ahmed.nafidi@uhp.ac.ma
Publikováno v:
Moroccan Journal of Pure & Applied Analysis. Oct2022, Vol. 8 Issue 3, p364-374. 11p.
Autor:
Per Hammarström
Publikováno v:
Nordisk Judaistik, Vol 35, Iss 1 (2024)
Recension av boken Plats i staden: Göteborgs judiska artonhundratal (Bokförlaget Korpen, 2023)
Externí odkaz:
https://doaj.org/article/6d7ea62ff4554ab6bc18f32bb1918970
Autor:
Nafidi, Ahmed, El Azri, Abdenbi
Publikováno v:
In Mathematics and Computers in Simulation April 2021 182:25-38
Autor:
Fu, Scarlet (AUTHOR), Bhasin, Kim (AUTHOR)
Publikováno v:
Bloomberg.com. 4/13/2023, pN.PAG-N.PAG. 1p.
Publikováno v:
Journal of Agricultural Sciences / Tarim Bilimleri Dergisi. 2021, Vol. 27 Issue 1, p1-8. 8p.
Akademický článek
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Autor:
Kling, Filip Jonsson, Lundqvist, Samuel, Mohammadi, Fatemeh, Orth, Matthias, Sáenz-de-Cabezón, Eduardo
For the almost complete intersection ideals $(x_1^2, \dots, x_n^2, (x_1 + \cdots + x_n)^k)$, we compute their reduced Gr\"obner basis for any term ordering, revealing a combinatorial structure linked to lattice paths, elementary symmetric polynomials
Externí odkaz:
http://arxiv.org/abs/2411.10209
Autor:
Venkattu, Deepika, Lundqvist, Peter, Torres, Miguel Pérez, Bonnassieux, Etienne, Tasse, Cyril, Melchior, Anne-Laure, Combes, Francoise
We present the first LOFAR image of the centre of M31 at a frequency of 150 MHz. We clearly detect three supernova remnants, which, along with archival VLA data at 3 GHz and other published radio and X-ray data allows us to characterize them in detai
Externí odkaz:
http://arxiv.org/abs/2410.22073
[SHORTENED VERSION] Observations of radio emission from young core-collapse supernovae (CCSNe) allow one to study the history of the pre-supernova stellar wind, trace the density structure of the ejected material, and probe the magnetohydrodynamics t
Externí odkaz:
http://arxiv.org/abs/2410.07800
Autor:
Salmaso, I., Cappellaro, E., Tartaglia, L., Anderson, J. P., Benetti, S., Bronikowski, M., Cai, Y. -Z., Charalampopoulos, P., Chen, T. -W., Concepcion, E., Elias-Rosa, N., Galbany, L., Gromadzki, M., Gutiérrez, C. P., Kankare, E., Lundqvist, P., Matilainen, K., Mazzali, P. A., Moran, S., Müller-Bravo, T. E., Nicholl, M., Pastorello, A., Pessi, P. J., Pessi, T., Petrushevska, T., Pignata, G., Reguitti, A., Sollerman, J., Srivastav, S., Stritzinger, M., Tomasella, L., Valerin, G.
Massive stars experience strong mass-loss, producing a dense, H-rich circumstellar medium (CSM). After the explosion, the collision and continued interaction of the supernova (SN) ejecta with the CSM power the light curve through the conversion of ki
Externí odkaz:
http://arxiv.org/abs/2410.06111