Zobrazeno 1 - 10
of 2 313
pro vyhledávání: '"Vries, B."'
Autor:
Royer, P., Merle, T., Dsilva, K., Sekaran, S., Van Winckel, H., Frémat, Y., Van der Swaelmen, M., Gebruers, S., Tkachenko, A., Laverick, M., Dirickx, M., Raskin, G., Hensberge, H., Abdul-Masih, M., Acke, B., Alonso, M. L., Mahato, S. Bandhu, Beck, P. G., Behara, N., Bloemen, S., Buysschaert, B., Cox, N., Debosscher, J., De Cat, P., Degroote, P., De Nutte, R., De Smedt, K., de Vries, B., Dumortier, L., Escorza, A., Exter, K., Goriely, S., Gorlova, N., Hillen, M., Homan, W., Jorissen, A., Kamath, D., Karjalainen, M., Karjalainen, R., Lampens, P., Lobel, A., Lombaert, R., Marcos-Arenal, P., Menu, J., Merges, F., Moravveji, E., Nemeth, P., Neyskens, P., Ostensen, R., Pápics, P. I., Perez, J., Royer, S. Prins S., Samadi-Ghadim, A., Sana, H., Fuentes, A. Sans, Scaringi, S., Schmid, V., Siess, L., Siopis, C., Smolders, K., Sodor, S., Thoul, A., Triana, S., Vandenbussche, B., Van de Sande, M., Van De Steene, G., Van Eck, S., van Hoof, P. A. M., Van Marle, A. J., Van Reeth, T., Vermeylen, L., Volpi, D., Vos, J., Waelkens, C.
Publikováno v:
A&A 681, A107 (2024)
Over the past decades, libraries of stellar spectra have been used in a large variety of science cases, including as sources of reference spectra for a given object or a given spectral type. Despite the existence of large libraries and the increasing
Externí odkaz:
http://arxiv.org/abs/2311.02705
Autor:
Luijken, K., Lohmann, A., Alter, U., Gonzalez, J. Claramunt, Clouth, F. J., Fossum, J. L., Hesen, L., Huizing, A. H. J., Ketelaar, J., Montoya, A. K., Nab, L., Nijman, R. C. C., de Vries, B. B. L. Penning, Tibbe, T. D., Wang, Y. A., Groenwold, R. H. H.
Results of simulation studies evaluating the performance of statistical methods are often considered actionable and thus can have a major impact on the way empirical research is implemented. However, so far there is limited evidence about the reprodu
Externí odkaz:
http://arxiv.org/abs/2307.02052
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Harknett, J., Whitworth, M., Rust, D., Krokos, M., Kearl, M., Tibaldi, A., Bonali, F.L., Van Wyk de Vries, B., Antoniou, V., Nomikou, P., Reitano, D., Falsaperla, S., Vitello, F., Becciani, U.
Publikováno v:
In Journal of Structural Geology October 2022 163
Publikováno v:
Published in Icarus: https://doi.org/10.1016/j.icarus.2017.10.029
Meteorites contain minerals from Solar System asteroids with different properties (like size, presence of water, core formation). We provide new mid-IR transmission spectra of powdered meteorites to obtain templates of how mid-IR spectra of asteroida
Externí odkaz:
http://arxiv.org/abs/1711.11306
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Lombaert, R., Decin, L., de Koter, A., Blommaert, J. A. D. L., Royer, P., De Beck, E., de Vries, B. L., Khouri, T., Min, M.
Publikováno v:
Astronomy & Astrophysics, 2013, Volume 554, id. A142, 19 pp
Context: AGB stars lose a large percentage of their mass in a dust-driven wind. This creates a circumstellar envelope, which can be studied through thermal dust emission and molecular emission lines. In the case of high mass-loss rates, this study is
Externí odkaz:
http://arxiv.org/abs/1505.07696
Autor:
Liseau, R., Larsson, B., Lunttila, T., Olberg, M., Rydbeck, G., Bergman, P., Justtanont, K., Olofsson, G., de Vries, B. L.
We aim at determining the spatial distribution of the gas and dust in star-forming regions and address their relative abundances in quantitative terms. We also examine the dust opacity exponent beta for spatial and/or temporal variations. Using mappi
Externí odkaz:
http://arxiv.org/abs/1504.06277
Autor:
Khouri, T., Waters, L. B. F. M., de Koter, A., Decin, L., Min, M., de Vries, B. L., Lombaert, R., Cox, N. L. J.
Publikováno v:
A&A 577, A114 (2015)
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:
http://arxiv.org/abs/1503.04765
Publikováno v:
A&A 578, A40 (2015)
We aim to constrain the structure of the circumstellar material around the post-AGB binary and RV Tauri pulsator AC Her. We want to constrain the spatial distribution of the amorphous as well as of the crystalline dust. We present very high-quality m
Externí odkaz:
http://arxiv.org/abs/1503.03984