Articles dans des revues avec comité de lecture (212)

  1. 79. Cruzalèbes, P., Jorissen, A., Rabbia, Y., Sacuto, S., Chiavassa, A., Pasquato, E., Plez, B., Eriksson, K. M., Spang, A., & Chesneau, O. (2013). Fundamental parameters of 16 late-type stars derived from their angular diameter measured with VLTI/AMBER. Monthly notices of the Royal Astronomical Society, 434, 437-450.
  2. 80. Dermine, T., Izzard, R., Jorissen, A., & Van Winckel, H. (2013). Erratum: Eccentricity-pumping in post-AGB stars with circumbinary discs (Astronomy and Astrophysics). Astronomy & astrophysics, 551, A50. doi:10.1051/0004-6361/201219430
  3. 81. Xu, Y., Goriely, S., Jorissen, A., Chen, G., & Arnould, M. (2013). Databases and tools for nuclear astrophysics applications: BRUSsels Nuclear LIBrary (BRUSLIB), Nuclear Astrophysics Compilation of REactions II (NACRE II) and Nuclear NETwork GENerator (NETGEN). Astronomy & astrophysics, 549, A106, 10. doi:10.1051/0004-6361/201220537
  4. 82. Deschamps, R., Siess, L., Davis, P., & Jorissen, A. (2013). Critically-rotating accretors and non-conservative evolution in Algols. Astronomy & astrophysics, 557, A40, 16.
  5. 83. Mayer, A., Jorissen, A., Kerschbaum, F., Ottensamer, R., Nowotny, W., Cox, N. L. J., Aringer, B., Blommaert, J., Decin, L., Van Eck, S., Gail, H.-P., Groenewegen, M. A. T., Kornfeld, K., Mecina, M., Posch, T., Vandenbussche, B., & Waelkens, C. (2013). Large-scale environments of binary AGB stars probed by Herschel. I. Morphology statistics and case studies of R Aquarii and W Aquilae. Astronomy & Astrophysics, 549, A69, 14. doi:10.1051/0004-6361/201219259
  6. 84. Paladini, C., Sacuto, S., Klotz, D., Ohnaka, K., Wittkowski, M., Nowotny, W., Jorissen, A., & Hron, J. (2012). Detection of an asymmetry in the envelope of the carbon Mira R Fornacis using VLTI/MIDI. Astronomy & astrophysics, 544, L5.
  7. 85. 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., Posch, T., Vandenbussche, B., & Waelkens, C. (2012). A far-infrared survey of bow shocks and detached shells around AGB stars and red supergiants (Corrigendum). Astronomy & Astrophysics, 543, C1. doi:10.1051/0004-6361/201117910e
  8. 86. Gorlova, N., Van Winckel, H., Gielen, C., Raskin, G., Prins, S., Pessemier, W., Waelkens, C., Frémat, Y., Hensberge, H., Dumortier, L., Jorissen, A., & Van Eck, S. (2012). Time-resolved spectroscopy of BD+46deg442: Gas streams and jet creation in a newly discovered evolved binary with a disk. Astronomy & astrophysics, 542, A27, 16. doi:10.1051/0004-6361/201118727
  9. 87. Bloemen, S., Marsh, T., Degroote, P., Ostensen, R., Pápics, P., Aerts, C., Koester, D., Gansicke, B., Breedt, E., Lombaert, R., Pyrzas, S., Copperwheat, C., Exter, K., Raskin, G., Van Winckel, H., Prins, S., Pessemier, W., Frémat, Y., Hensberge, H., Jorissen, A., & Van Eck, S. (2012). Mass ratio from Doppler beaming and Romer delay versus ellipsoidal modulation in the Kepler data of KOI-74. Monthly notices of the Royal Astronomical Society, 422, 2600-2608. doi:10.1111/j.1365-2966.2012.20818.x
  10. 88. Wahlgren, G., van Dishoeck, E., Federman, S., Beiersdorfer, P., Dimitrijevic, M., Jorissen, A., Mashonkina, L., Nilsson, H., Salama, F., & Tennyson, J. (2012). Commission 14: Atomic and Molecular Data. Transactions of the International Astronomical Union, 28, 339-340. doi:10.1017/S1743921312003079
  11. 89. Jorissen, A., Van Eck, S., Dermine, T., Van Winckel, H., & Gorlova, N. (2012). New symbiotic stars monitored with the HERMES spectrograph: A case study of orbital ha modulation. Baltic astronomy, 21(1-2), 37-44.
  12. 90. Paladini, C., Klotz, D., Hron, J., Kerschbaum, F., Sacuto, S., Wittkowski, M., Lagadec, E., Verhoelst, T., Jorissen, A., Richichi, A., Groenewegen, M. A. T., & Olofsson, H. (2012). To be or not to be asymmetric? VLTI and the mass loss geometry of red giants. Proceedings of SPIE - The International Society for Optical Engineering, 8445, 84451R. doi:10.1117/12.926380

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