Zobrazeno 1 - 10
of 386
pro vyhledávání: '"Anthonioz P"'
Autor:
Greg Woolf
Publikováno v:
Arys. Antigüedad, Religiones y Sociedades, Iss 19 (2021)
Externí odkaz:
https://doaj.org/article/d0068bbde1154ba683699576f3bb4a9f
Autor:
Foster, Benjamin R.
Publikováno v:
Orientalistische Literaturzeitung; July 2022, Vol. 117 Issue: 2 p113-116, 4p
Autor:
Dionatos, O., Woitke, P., Guedel, M., Degroote, P., Liebhart, A., Anthonioz, F., Antonellini, S., Baldovin-Saavedra, C., Carmona, A., Dominik, C., Greaves, J., Ilee, J. D., Kamp, I., Menard, F., Min, M., Pinte, C., Rab, C., Rigon, L., Thi, W. F., Waters, L. B. F. M.
Publikováno v:
A&A 625, A66 (2019)
Consistent modeling of protoplanetary disks requires the simultaneous solution of both continuum and line radiative transfer, heating/cooling balance between dust and gas and, of course, chemistry. Such models depend on panchromatic observations that
Externí odkaz:
http://arxiv.org/abs/1902.11204
Autor:
Woitke, P., Kamp, I., Antonellini, S., Anthonioz, F., Baldovin-Saveedra, C., Carmona, A., Dionatos, O., Dominik, C., Greaves, J., Güdel, M., Ilee, J. D., Liebhardt, A., Menard, F., Min, M., Pinte, C., Rab, C., Rigon, L., Thi, W. -F., Thureau, N., Waters, L. B. F. M.
The European FP7 project DIANA has performed a coherent analysis of a large set of observations from protoplanetary disks by means of thermo-chemical disk models. The collected data include extinction-corrected stellar UV and X-ray input spectra (as
Externí odkaz:
http://arxiv.org/abs/1812.02741
Autor:
Bouquin, J. -B. Le, Sana, H., Gosset, E., De Becker, M., Duvert, G., Absil, O., Anthonioz, F., Berger, J. -P., Ertel, S., Grellmann, R., Guieu, S., Kervella, P., Rabus, M., Willson, M.
Publikováno v:
A&A 601, A34 (2017)
Our long term aim is to derive model-independent stellar masses and distances for long period massive binaries by combining apparent astrometric orbit with double-lined radial velocity amplitudes (SB2). We follow-up ten O+O binaries with AMBER, PIONI
Externí odkaz:
http://arxiv.org/abs/1608.03525
Autor:
Woitke, P., Min, M., Pinte, C., Thi, W. -F., Kamp, I., Rab, C., Anthonioz, F., Antonellini, S., Baldovin-Saavedra, C., Carmona, A., Dominik, C., Dionatos, O., Greaves, J., Güdel, M., Ilee, J. D., Liebhart, A., Ménard, F., Rigon, L., Waters, L. B. F. M., Aresu, G., Meijerink, R., Spaans, M.
Publikováno v:
A&A 586, A103 (2016)
We propose a set of standard assumptions for the modelling of Class II and III protoplanetary disks, which includes detailed continuum radiative transfer, thermo-chemical modelling of gas and ice, and line radiative transfer from optical to cm wavele
Externí odkaz:
http://arxiv.org/abs/1511.03431
Autor:
Halbwachs, J. -L., Boffin, H. M. J., Bouquin, J. -B. Le, Kiefer, F., Famaey, B., Salomon, J. -B., Arenou, F., Pourbaix, D., Anthonioz, F., Grellmann, R., Guieu, S., Sana, H., Guillout, P., Jorissen, A., Lebreton, Y., Mazeh, T., Tal-Or, L., Gomez-Moran, A. Nebot
In anticipation of the Gaia astrometric mission, a sample of spectroscopic binaries is being observed since 2010 with the Sophie spectrograph at the Haute--Provence Observatory. Our aim is to derive the orbital elements of double-lined spectroscopic
Externí odkaz:
http://arxiv.org/abs/1510.07412
Autor:
Anthonioz, Fabien, Ménard, François, Pinte, Christophe, Bouquin, Jean-Baptiste Le, Benisty, Myriam, Thi, Wing-Fai, Absil, Olivier, Duchêne, Gaspard, Augereau, Jean-Charles, Berger, Jean-Phillipe, Casassus, Simon, Duvert, Gilles, Lazareff, Bernard, Malbet, Fabien, Millan-Gabet, Rafael, Schreiber, Matthias R., Traub, Wesley, Zins, Gérard
Publikováno v:
A&A 574, A41 (2015)
Context : The properties of the inner disks of bright Herbig AeBe stars have been studied with near infrared (NIR) interferometry and high resolution spectroscopy. The continuum and a few molecular gas species have been studied close to the central s
Externí odkaz:
http://arxiv.org/abs/1412.1052
Akademický článek
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Autor:
Alberola, N., Anthonioz, T., Badertscher, A., Bas, C., Belov, A. S., Crivelli, P., Gninenko, S. N., Golubev, N. A., Kirsanov, M. M., Rubbia, A., Sillou, D.
Publikováno v:
Nucl.Instrum.Meth.A560:224-232,2006
We have developed a high-efficiency pulsed slow positron beam for experiments with orthopositronium in vacuum. The new pulsing scheme is based on a double-gap coaxial buncher powered by an RF pulse of appropriate shape. The modulation of the positron
Externí odkaz:
http://arxiv.org/abs/physics/0511048