Zobrazeno 1 - 10
of 278
pro vyhledávání: '"van Marle, A. J."'
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:
Chrimes, A. A., Gompertz, B. P., Kann, D. A., van Marle, A. J., Eldridge, J. J., Groot, P. J., Laskar, T., Levan, A. J., Nicholl, M., Stanway, E. R., Wiersema, K.
The temporal and spectral evolution of gamma-ray burst (GRB) afterglows can be used to infer the density and density profile of the medium through which the shock is propagating. In long-duration (core-collapse) GRBs, the circumstellar medium (CSM) i
Externí odkaz:
http://arxiv.org/abs/2206.13595
Akademický článek
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Akademický článek
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Massive stars that have been ejected from their parent cluster and supersonically sailing away through the interstellar medium (ISM) are classified as exiled. They generate circumstellar bow shock nebulae that can be observed. We present two-dimensio
Externí odkaz:
http://arxiv.org/abs/1603.04755
Autor:
van Minnen, Agnes, Vos, Lizelotte, Bet, Pierre M., de Jongh, Ad, Linsen, Felix, van Marle, Hein J. F., Meijer, Onno C., Otte, Willem M., Russcher, Marije, Vinkers, Christiaan H.
Publikováno v:
Case Reports in Psychiatry; 4/26/2024, Vol. 2024, p1-6, 6p
Publikováno v:
A&A 570, A131 (2014)
We aim to examine the role of the interstellar magnetic field in shaping the extended morphologies of slow dusty winds of Asymptotic Giant-branch (AGB) stars in an effort to pin-point the origin of so-called eye shaped CSE of three carbon-rich AGB st
Externí odkaz:
http://arxiv.org/abs/1408.1510
Autor:
Beck, P. G., Hambleton, K., Vos, J., Kallinger, T., Bloemen, S., Tkachenko, A., García, R. A., Østensen, R. H., Aerts, C., Kurtz, D. W., De Ridder, J., Hekker, S., Pavlovski, K., Mathur, S., De Smedt, K., Derekas, A., Corsaro, E., Mosser, B., Van Winckel, H., Huber, D., Degroote, P., Davies, G. R., Prša, A., Debosscher, J., Elsworth, Y., Nemeth, P., Siess, L., Schmid, V. S., Pápics, P. I., de Vries, B. L., van Marle, A. J., Marcos-Arenal, P., Lobel, A.
The unparalleled photometric data obtained by NASA's Kepler space telescope led to an improved understanding of red giant stars and binary stars. Seismology allows us to constrain the properties of red giants. In addition to eclipsing binaries, eccen
Externí odkaz:
http://arxiv.org/abs/1312.4500
Autor:
Decin, L., Cox, N. L. J., Royer, P., Van Marle, A. J., Vandenbussche, B., Ladjal, D., Kerschbaum, F., Ottensamer, R., Barlow, M. J., Blommaert, J. A. D. L., Gomez, H. L., Groenewegen, M. A. T., Lim, T., Swinyard, B. M., Waelkens, C., Tielens, A. G. G. M.
Publikováno v:
2012, Astronomy and Astrophysics, 548, A113
Context. The interaction between stellar winds and the interstellar medium (ISM) can create complex bow shocks. The photometers on board the Herschel Space Observatory are ideally suited to studying the morphologies of these bow shocks. Aims. We aim
Externí odkaz:
http://arxiv.org/abs/1212.4870
Autor:
Cox, N. L. J., Kerschbaum, F., van Marle, A. -J., Decin, L., Ladjal, D., Mayer, A., Groenewegen, M. A. T., van Eck, S., Royer, P., Ottensamer, R., Ueta, T., Jorissen, A., Mecina, M., Meliani, Z., Luntzer, A., Blommaert, J. A. D. L., Posch, Th., Vandenbussche, B., Waelkens, C.
Far-infrared Herschel/PACS images at 70 and 160 micron of a sample of 78 Galactic evolved stars are used to study the (dust) emission structures, originating from stellar wind-ISM interaction. In addition, two-fluid hydrodynamical simulations of the
Externí odkaz:
http://arxiv.org/abs/1110.5486