Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Monsalvo, I. de Gregorio"'
Autor:
Testi, L., Natta, A., Manara, C. F., Monsalvo, I. de Gregorio, Lodato, G., Lopez, C., Muzic, K., Pascucci, I., Sanchis, E., Miranda, A. Santamaria, Scholz, A., De Simone, M., Williams, J. P.
Publikováno v:
A&A 663, A98 (2022)
(Abridged) We present a study of the disk population in L1688, the densest and youngest region in Ophiuchus, and we compare it with other nearby regions of different age, namely Lupus, Chamaeleon I, Corona Australis, Taurus and Upper Scorpius. We sel
Externí odkaz:
http://arxiv.org/abs/2201.04079
Autor:
Sánchez-Ramírez, R., Hancock, P. J., Jóhannesson, G., Murphy, Tara, Postigo, A. de Ugarte, Gorosabel, J., Kann, D. A., Krühler, T., Oates, S. R., Japelj, J., Thöne, C. C., Lundgren, A., Perley, D. A., Malesani, D., Monsalvo, I. de Gregorio, Castro-Tirado, A. J., D'Elia, V., Fynbo, J. P. U., Garcia-Appadoo, D., Goldoni, P., Greiner, J., Hu, Y. -D., Jelínek, M., Jeong, S., Kamble, A., Klose, S., Kuin, N. P. M., Llorente, A., Martín, S., Guelbenzu, A. Nicuesa, Rossi, A., Schady, P., Sparre, M., Sudilovsky, V., Tello, J. C., Updike, A., Wiersema, K., Zhang, B. -B.
Publikováno v:
MNRAS, 464, 4624 (2017)
We present the extensive follow-up campaign on the afterglow of GRB 110715A at 17 different wavelengths, from X-ray to radio bands, starting 81 seconds after the burst and extending up to 74 days later. We performed for the first time a GRB afterglow
Externí odkaz:
http://arxiv.org/abs/1610.01844
Publikováno v:
A&A 593, A111 (2016)
The study of the properties of disks around young brown dwarfs can provide important clues on the formation of these very low-mass objects and on the possibility of forming planetary systems around them. The presence of warm dusty disks around brown
Externí odkaz:
http://arxiv.org/abs/1606.06448
Autor:
Postigo, A. de Ugarte, Lundgren, A., Martín, S., Garcia-Appadoo, D., Monsalvo, I. de Gregorio, Peck, A., Michałowski, M. J., Thöne, C. C., Campana, S., Gorosabel, J., Tanvir, N. R., Wiersema, K., Castro-Tirado, A. J., Schulze, S., De Breuck, C., Petitpas, G., Hjorth, J., Jakobsson, P., Covino, S., Fynbo, J. P. U., Winters, J. M., Bremer, M., Levan, A. J., Llorente, A., Sánchez-Ramírez, R., Tello, J. C., Salvaterra, R.
GRBs generate an afterglow emission that can be detected from radio to X-rays during days, or even weeks after the initial explosion. The peak of this emission crosses the mm/submm range during the first hours to days, making their study in this rang
Externí odkaz:
http://arxiv.org/abs/1108.1797