Zobrazeno 1 - 10
of 3 085
pro vyhledávání: '"Duran R."'
Publikováno v:
In Science of the Total Environment 15 October 2024 947
Publikováno v:
In Geomorphology 15 September 2024 461
Autor:
Kamenetskaia, B. Betancourt, Fraija, N., Dainotti, M., Gálvan-Gámez, A., Duran, R. Barniol, Dichiara, S.
We investigate the evolution of the afterglow produced by the deceleration of the non-relativistic material due to its surroundings. The ejecta mass is launched into the circumstellar medium with equivalent kinetic energy expressed as a power-law vel
Externí odkaz:
http://arxiv.org/abs/2108.10811
Autor:
Kamenetskaia, B. Betancourt, Fraija, N., Dainotti, M., Gálvan-Gámez, A., Duran, R. Barniol, Dichiara, S.
In light of the most recent observations of late afterglows produced by the merger of compact objects or by the core-collapse of massive dying stars, we research the evolution of the afterglow produced by an off-axis top-hat jet and its interaction w
Externí odkaz:
http://arxiv.org/abs/2108.10797
Autor:
Lobo, F.J., dos Passos Nascimento, J.L., Durán, R., López-Quirós, A., Guillén, J., Pereira, F., Rocha, C.B., de Mahiques, M.M.
Publikováno v:
In Geomorphology 1 July 2024 456
Autor:
Cerrillo-Escoriza, J., Lobo, F.J., Puga-Bernabéu, Á., Bárcenas, P., Mendes, I., Pérez-Asensio, J.N., Durán, R., Andersen, T.J., Carrión-Torrente, Á., García, M., López-Quirós, A., Luján, M., Mena, A., Sánchez-Guillamón, O., Sánchez, M.J.
Publikováno v:
In Geomorphology 15 May 2024 453
Autor:
Stroh, M. C., Terreran, G., Coppejans, D. L., Bright, J. S., Margutti, R., Bietenholz, M. F., De Colle, F., DeMarchi, L., Duran, R. Barniol, Milisavljevic, D., Murase, K., Paterson, K., Williams, W. L.
Publikováno v:
ApJL 923 (2021) L24
We present a population of 19 radio-luminous supernovae (SNe) with emission reaching $L_{\nu}{\sim}10^{26}-10^{29}\,\rm{erg\,s^{-1}Hz^{-1}}$ in the first epoch of the Very Large Array Sky Survey (VLASS) at $2-4$GHz. Our sample includes one long Gamma
Externí odkaz:
http://arxiv.org/abs/2106.09737
Autor:
Hajela, A., Margutti, R., Bright, J. S., Alexander, K. D., Metzger, B. D., Nedora, V., Kathirgamaraju, A., Margalit, B., Radice, D., Guidorzi, C., Berger, E., MacFadyen, A., Giannios, D., Chornock, R., Heywood, I., Sironi, L., Gottlieb, O., Coppejans, D., Laskar, T., Cendes, Y., Duran, R. Barniol, Eftekhari, T., Fong, W., McDowell, A., Nicholl, M., Xie, X., Zrake, J., Bernuzzi, S., Broekgaarden, F. S., Kilpatrick, C. D., Terreran, G., Villar, V. A., Blanchard, P. K., Gomez, S., Hosseinzadeh, G., Matthews, D. J., Rastinejad, J. C.
For the first $\sim3$ years after the binary neutron star merger event GW 170817 the radio and X-ray radiation has been dominated by emission from a structured relativistic off-axis jet propagating into a low-density medium with n $< 0.01\,\rm{cm^{-3
Externí odkaz:
http://arxiv.org/abs/2104.02070
Autor:
Fraija, N., Laskar, T., Dichiara, S., Beniamini, P., Duran, R. Barniol, Dainotti, M. G., Becerra, R. L.
The Fermi-LAT collaboration presented the second gamma-ray burst (GRB) catalog covering its first 10 years of operations. A significant fraction of afterglow-phase light curves in this catalog cannot be explained by the closure relations of the stand
Externí odkaz:
http://arxiv.org/abs/2006.10291
The central engine in long gamma-ray bursts (GRBs) is thought to be a compact object produced by the core collapse of massive stars, but its exact nature (black hole or millisecond magnetar) is still debatable. Although the central engine of GRB coll
Externí odkaz:
http://arxiv.org/abs/2006.07482