Zobrazeno 1 - 10
of 14
pro vyhledávání: '"H. Boussier"'
Autor:
M. Vrašťák, F. Sims, P. Velez, T. Bohlsen, F. Teyssier, C. Boussin, Marek Wolf, J. Merc, H. Boussier, P. Cazzato, C. Buil, I Diarrasouba, Rudolf Gális
Symbiotic stars belong to a group of interacting binaries that display a wide variety of phenomena, including prominent outbursts connected with mass transfer, as well as stellar winds, jets, eclipses, or intrinsic variability of the components. Doze
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c20f7f0c4714207b61c1847560ee528a
Autor:
M. Banfi, Simona Ciceri, C. Kotnik, S. Vanaverbeke, Matthias Mallonn, Christopher A. Watson, John Briol, H. Boussier, Joseph E. Rodriguez, P. Lewin, S. P. Littlefair, Elizabeth O. Waagen, D. W. Latham, Matthew A. Kenworthy, Alexander Scholz, F. Dubois, Edward Gomez, Richard Wilson, Gabriel Murawski, R. Papini, T. Killestein, Mike Calkins, Rafael Sfair, H. Relles, Matthew R. Burleigh, E. Dose, R. Jayawardhana, U. Quadri, G. Zhou, Peter J. Wheatley, C. Lopresti, M. Hippke, E. J. W. de Mooij, S. Kafka, Richard G. West, Jeff W. Robertson, Grant M. Kennedy, S. Dvorak, G. Myers, Liam Raynard, V. S. Dhillon, Daniel F. Evans, L. Rizzuti, P. Benni, Alessandro Marchini, J. McCormac, Maximilian N. Günther, S. N. Quinn, Timothy Butterley, K. Hills, Luigi Mancini, S. M. Brincat, Alexis M. S. Smith, L. Barbieri, R. James, Perry Berlind, I. S. Becker, Allyson Bieryla, M. Deldem, S. Ferratfiat, John Southworth, Velimir A. Popov, P. Chote, F.-J. Hambsch, E. Herrero, Othon C. Winter, S. J. Fossey, G. Bonnoli, D. Lemay, J. Hall, F. Salvaggio, Hugh P. Osborn, Gil Esquerdo, Thiam-Guan Tan
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2019, 485, pp.1614-1625. ⟨10.1093/mnras/stz283⟩
Monthly Notices of the RAS (0035-8711), 485(2), 1614-1625
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Monthly notices of the Royal Astronomical Society, 2019, Vol.485(2), pp.1614-1625 [Peer Reviewed Journal]
Osborn, H P, Kenworthy, M, Rodriguez, J E, de Mooij, E J W, Kennedy, G M, Relles, H, Gomez, E, Hippke, M, Banfi, M, Barbieri, L, Becker, I S, Benni, P, Berlind, P, Bieryla, A, Bonnoli, G, Boussier, H, Brincat, S M, Briol, J, Burleigh, M R, Butterley, T, Calkins, M L, Chote, P, Ciceri, S, Deldem, M, Dhillon, V S, Dose, E, Dubois, F, Dvorak, S, Esquerdo, G A, Evans, D F, Ferratfiat, S, Fossey, S J, Günther, M N, Hall, J, Hambsch, F-J, Herrero, E, Hills, K, James, R, Jayawardhana, R, Kafka, S, Killestein, T L, Kotnik, C, Latham, D W, Lemay, D, Lewin, P, Littlefair, S, Lopresti, C, Mallonn, M, Mancini, L, Marchini, A, McCormac, J J, Murawski, G, Myers, G, Papini, R, Popov, V, Quadri, U, Quinn, S N, Raynard, L, Rizzuti, L, Robertson, J, Salvaggio, F, Scholz, A, Sfair, R, Smith, A M S, Southworth, J, Tan, T G, Vanaverbeke, S, Waagen, E O, Watson, C A, West, R G, Winter, O C, Wheatley, P J, Wilson, R W & Zhou, G 2019, ' The PDS 110 observing campaign-photometric and spectroscopic observations reveal eclipses are aperiodic ', Monthly Notices of the Royal Astronomical Society, Advance Access . https://doi.org/10.1093/mnras/stz283
Monthly Notices of the Royal Astronomical Society, 2019, 485, pp.1614-1625. ⟨10.1093/mnras/stz283⟩
Monthly Notices of the RAS (0035-8711), 485(2), 1614-1625
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Monthly notices of the Royal Astronomical Society, 2019, Vol.485(2), pp.1614-1625 [Peer Reviewed Journal]
Osborn, H P, Kenworthy, M, Rodriguez, J E, de Mooij, E J W, Kennedy, G M, Relles, H, Gomez, E, Hippke, M, Banfi, M, Barbieri, L, Becker, I S, Benni, P, Berlind, P, Bieryla, A, Bonnoli, G, Boussier, H, Brincat, S M, Briol, J, Burleigh, M R, Butterley, T, Calkins, M L, Chote, P, Ciceri, S, Deldem, M, Dhillon, V S, Dose, E, Dubois, F, Dvorak, S, Esquerdo, G A, Evans, D F, Ferratfiat, S, Fossey, S J, Günther, M N, Hall, J, Hambsch, F-J, Herrero, E, Hills, K, James, R, Jayawardhana, R, Kafka, S, Killestein, T L, Kotnik, C, Latham, D W, Lemay, D, Lewin, P, Littlefair, S, Lopresti, C, Mallonn, M, Mancini, L, Marchini, A, McCormac, J J, Murawski, G, Myers, G, Papini, R, Popov, V, Quadri, U, Quinn, S N, Raynard, L, Rizzuti, L, Robertson, J, Salvaggio, F, Scholz, A, Sfair, R, Smith, A M S, Southworth, J, Tan, T G, Vanaverbeke, S, Waagen, E O, Watson, C A, West, R G, Winter, O C, Wheatley, P J, Wilson, R W & Zhou, G 2019, ' The PDS 110 observing campaign-photometric and spectroscopic observations reveal eclipses are aperiodic ', Monthly Notices of the Royal Astronomical Society, Advance Access . https://doi.org/10.1093/mnras/stz283
PDS 110 is a young disk-hosting star in the Orion OB1A association. Two dimming events of similar depth and duration were seen in 2008 (WASP) and 2011 (KELT), consistent with an object in a closed periodic orbit. In this paper we present data from a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::568c8cdceec7e7a5b9d35621baaf28ef
https://hal-insu.archives-ouvertes.fr/insu-03666751/document
https://hal-insu.archives-ouvertes.fr/insu-03666751/document
Autor:
Jacques Crovisier, Dominique Bockelée-Morvan, Gabriel Paubert, Raphael Moreno, E. Bertrand, Jérémie Boissier, Nicolas Biver, Michael A. DiSanti, H. Boussier, Adam J. McKay, N. Dello Russo, F. Kugel
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 619, pp.A127. ⟨10.1051/0004-6361/201833449⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 619, pp.A127. ⟨10.1051/0004-6361/201833449⟩
We present a multi-wavelength study of comet C/2016 R2 (PanSTARRS). This comet was observed on 23-24 January 2018 with the IRAM 30m telescope, and in January to March 2018 with the Nan\c{c}ay radio telescope. Visible spectroscopy was performed in Dec
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::098f70e3a7cb8e22daf1e57f70707953
https://hal.archives-ouvertes.fr/hal-02300995
https://hal.archives-ouvertes.fr/hal-02300995
Autor:
F. Peron, H. Boussier
Publikováno v:
Procedia Chemistry. 7:740-745
The reference pyrochemistry process studied by the DRCP is based on an actinide reductive extraction in fluoride media. At the front end of the process, a hydrofluorination step is needed in order to convert the oxides present in irradiated fuel into
Autor:
A. Santerne, G. Hébrard, J. Lillo-Box, D. J. Armstrong, S. C. C. Barros, O. Demangeon, D. Barrado, A. Debackere, M. Deleuil, E. Delgado Mena, M. Montalto, D. Pollacco, H. P. Osborn, S. G. Sousa, L. Abe, V. Adibekyan, J.-M. Almenara, P. André, G. Arlic, G. Barthe, P. Bendjoya, R. Behrend, I. Boisse, F. Bouchy, H. Boussier, M. Bretton, D. J. A. Brown, B. Carry, A. Cailleau, E. Conseil, G. Coulon, B. Courcol, B. Dauchet, J.-C. Dalouzy, M. Deldem, O. Desormières, P. Dubreuil, J.-M. Fehrenbach, S. Ferratfiat, R. Girelli, J. Gregorio, S. Jaecques, F. Kugel, J. Kirk, O. Labrevoir, J.-C. Lachurié, K. W. F. Lam, P. Le Guen, P. Martinez, L. P. A. Maurin, J. McCormac, J-B. Pioppa, U. Quadri, A. Rajpurohit, J. Rey, J.-P. Rivet, R. Roy, N. C. Santos, F. Signoret, L. Strabla, O. Suarez, D. Toublanc, M. Tsantaki, J.-M. Vienney, P. A. Wilson, M. Bachschmidt, F. Colas, O. Gerteis, P. Louis, J.-C. Mario, C. Marlot, J. Montier, V. Perroud, V. Pic, D. Romeuf, S. Ubaud, D. Verilhac
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2016, 824 (1), ⟨10.3847/0004-637X/824/1/55⟩
Astrophysical Journal
Astrophysical Journal, American Astronomical Society, 2016, 824 (1), 〈10.3847/0004-637X/824/1/55〉
The Astrophysical Journal, 2016, 824 (1), ⟨10.3847/0004-637X/824/1/55⟩
The Astrophysical Journal, American Astronomical Society, 2016, 824 (1), ⟨10.3847/0004-637X/824/1/55⟩
Astrophysical Journal
Astrophysical Journal, American Astronomical Society, 2016, 824 (1), 〈10.3847/0004-637X/824/1/55〉
The Astrophysical Journal, 2016, 824 (1), ⟨10.3847/0004-637X/824/1/55⟩
International audience; In the present paper we report the discovery of a new hot Jupiter, K2-29 b, first detected by the Super-WASP observatory and then by the K2 space mission during its campaign 4. The planet has a period of 3.25 days, a mass of 0
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