Zobrazeno 1 - 10
of 353
pro vyhledávání: '"Juhász, Attila"'
Autor:
Ádány, Róza1,2,3,4 (AUTHOR) adany.roza@med.unideb.hu, Juhász, Attila1 (AUTHOR) nagy.csilla@semmelweis.hu, Nagy, Csilla1 (AUTHOR) burkali.bernadett@semmelweis.hu, Burkali, Bernadett1,5 (AUTHOR) piko.peter@semmelweis.hu, Pikó, Péter1,2 (AUTHOR) oroszi.beatrix@semmelweis.hu, McKee, Martin6 (AUTHOR) martin.mckee@lshtm.ac.uk, Oroszi, Beatrix1 (AUTHOR)
Publikováno v:
Cancers. Aug2024, Vol. 16 Issue 16, p2917. 20p.
Autor:
Juhász, Attila1 juhasz.attila@emk.bme.hu, Balogh, Árpád1,2 balogh.arpad@emk.bme.hu
Publikováno v:
Geodetski Vestnik. 2024, Vol. 68 Issue 2, p211-222. 12p.
Annular structures in proto-planetary discs, such as gaps and rings, are now ubiquitously found by high-resolution ALMA observations. Under the hypothesis that they are opened by planets, in this paper we investigate how the minimum planet mass neede
Externí odkaz:
http://arxiv.org/abs/2002.11036
Autor:
Moór, Attila, Kral, Quentin, Ábrahám, Péter, Kóspál, Ágnes, Dutrey, Anne, di Folco, Emmanuel, Hughes, A. Meredith, Juhász, Attila, Pascucci, Ilaria, Pawellek, Nicole
Previous observations revealed the existence of CO gas at nearly protoplanetary level in several dust-rich debris disks around young A-type stars. Here we used the ALMA 7m-array to measure $^{13}$CO and C$^{18}$O emission toward two debris disks, 49
Externí odkaz:
http://arxiv.org/abs/1908.09685
Autor:
Nazari, Pooneh, Booth, Richard A., Clarke, Cathie J., Rosotti, Giovanni P., Tazzari, Marco, Juhasz, Attila, Meru, Farzana
Recent observations show that rings and gaps are ubiquitous in protoplanetary discs. These features are often interpreted as being due to the presence of planets; however, the effect of planetary migration on the observed morphology has not been inve
Externí odkaz:
http://arxiv.org/abs/1903.03114
Autor:
Clarke, Cathie J., Tazzari, Marco, Juhász, Attila, Rosotti, Giovanni, Booth, Richard, Facchini, Stefano, Ilee, John D., Johns-Krull, Christopher M., Kama, Mihkel, Meru, Farzana, Prato, Lisa
We present high resolution millimeter continuum imaging of the disc surrounding the young star CI Tau, a system hosting the first hot Jupiter candidate in a protoplanetary disc system. The system has extended mm emission on which are superposed three
Externí odkaz:
http://arxiv.org/abs/1809.08147
Autor:
Monnier, John D., Kraus, Stefan, Ireland, Michael J., Baron, Fabien, Bayo, Amelia, Berger, Jean-Philippe, Creech-Eakman, Michelle, Dong, Ruobing, Duchene, Gaspard, Espaillat, Catherine, Haniff, Chris, Honig, Sebastian, Isella, Andrea, Juhasz, Attila, Labadie, Lucas, Lacour, Sylvestre, Leifer, Stephanie, Merand, Antoine, Michael, Ernest, Minardi, Stefano, Mordasini, Christoph, Mozurkewich, David, Olofsson, Johan, Paladini, Claudia, Petrov, Romain, Pott, Jorg-Uwe, Ridgway, Stephen, Rinehart, Stephen, Stassun, Keivan, Surdej, Jean, Brummelaar, Theo ten, Turner, Neal, Tuthill, Peter, Vahala, Kerry, van Belle, Gerard, Vasisht, Gautam, Wishnow, Ed, Young, John, Zhu, Zhaohuan
Publikováno v:
Monnier, J.D., Kraus, S., Ireland, M.J. et al. Exp Astron (2018). https://doi.org/10.1007/s10686-018-9594-1
The Planet Formation Imager (PFI, www.planetformationimager.org) is a next-generation infrared interferometer array with the primary goal of imaging the active phases of planet formation in nearby star forming regions. PFI will be sensitive to warm d
Externí odkaz:
http://arxiv.org/abs/1807.11559
Autor:
Price, Daniel J., Cuello, Nicolas, Pinte, Christophe, Mentiplay, Daniel, Casassus, Simon, Christiaens, Valentin, Kennedy, Grant M., Cuadra, Jorge, M., Sebastian Perez, Marino, Sebastian, Armitage, Philip J., Zurlo, Alice, Juhasz, Attila, Ragusa, Enrico, Laibe, Guillaume, Lodato, Giuseppe
We present 3D hydrodynamical models of the HD142527 protoplanetary disc, a bright and well studied disc that shows spirals and shadows in scattered light around a 100 au gas cavity, a large horseshoe dust structure in mm continuum emission, together
Externí odkaz:
http://arxiv.org/abs/1803.02484
Publikováno v:
A&A 611, A16 (2018)
Sulphur-bearing volatiles are observed to be significantly depleted in interstellar and circumstellar regions. This missing sulphur is postulated to be mostly locked up in refractory form. With ALMA we have detected sulphur monoxide (SO), a known sho
Externí odkaz:
http://arxiv.org/abs/1712.05992
Autor:
Juhasz, Attila, Rosotti, Giovanni P.
Spiral arms have been observed in nearly a dozen protoplanetary discs in near-infrared scattered light and recently also in the sub-millimetre continuum. While one of the most compelling explanations is that they are driven by planetary or stellar co
Externí odkaz:
http://arxiv.org/abs/1711.03559