Zobrazeno 1 - 10
of 150
pro vyhledávání: '"Dagostino, M"'
Autor:
Rojas-García, O. S., Gómez-Ruiz, A. I., Palau, A., Orozco-Aguilera, M. T., Kurtz, S. E., Dagostino, M. Chavez
G351.16+0.70 is a relatively well-studied High Mass Star Forming Region with at least two main bipolar outflow structures originating from an OB embedded star and multiple IR cores. Using high-resolution and large bandwidth SMA observations, we studi
Externí odkaz:
http://arxiv.org/abs/2303.02527
Autor:
Rojas-García, O. S., Gómez-Ruiz, A. I., Palau, A., Orozco-Aguilera, M. T., Dagostino, M. Chavez, Kurtz, S. E.
The interstellar medium contains dust and gas, in which at high densities and cold conditions molecules can proliferate. Interstellar Complex Organic Molecules (iCOMs) are C-bearing species that contain at least six atoms. As they are detected in you
Externí odkaz:
http://arxiv.org/abs/2207.09426
Autor:
Piantelli, S., Casini, G., Ono, A., Poggi, G., Pastore, G., Barlini, S., Boiano, A., Bonnet, E., Borderie, B., Bougault, R., Bruno, M., Buccola, A., Camaiani, A., Chbihi, A., Cicerchia, M., Cinausero, M., DAgostino, M., Degerlier, M., Duenas, J., Fable, Q., Fabris, D., Frankland, J. D., Frosin, C., Gramegna, F., Gruyer, D., Henri, M., Kordyasz, A., Kozik, T., LeNeindre, N., Lombardo, I., Lopez, O., Mantovani, G., Marchi, T., Morelli, L., Olmi, A., Ottanelli, P., Parlog, M., Pasquali, G., Stefanini, A. A., Tortone, G., Upadhyaya, S., Valdre, S., Verde, G., Vient, E., Vigilante, M., Alba, R., Maiolino, C.
Publikováno v:
Physical Review C 101, 034613 (2020)
Experimental results concerning the dynamical fission of quasiprojectiles in semiperipheral collisions for the system 80 Kr+ 48 Ca at 35 MeV/nucleon are presented. Data have been collected with four blocks of the FAZIA setup in the first physics expe
Externí odkaz:
http://arxiv.org/abs/2010.00447
Autor:
Bognár, Zs., Paparó, M., Sódor, Á., Jenei, D. I., Kalup, Cs., Bertone, E., Chavez-Dagostino, M., Montgomery, M. H., Győrffy, Á., Molnár, L., Ollé, H., Pápics, P. I., Plachy, E., Verebélyi, E.
We summarize our findings on three cool ZZ Ceti type pulsating white dwarfs. We determined eight independent modes in HS 0733+4119, of which seven are new findings. For GD 154, we detected two new eigenmodes, and the recurrence of the pulsational beh
Externí odkaz:
http://arxiv.org/abs/1810.09711
Autor:
Gómez-Ruiz, A. I., Guzman-Ramirez, L., Serrano, E. O., Sanchez-Arguelles, D., Luna, A., Schloerb, F. P., Narayanan, G., Yun, M. S., Sahai, R., Zijlstra, A. A., Chavez-Dagostino, M., Montaña, A., Hughes, D. H., Rodríguez, M.
Extremely high velocity emission likely related to jets is known to occur in some proto-Planetary Nebulae. However, the molecular complexity of this kinematic component is largely unknown. We observed the known extreme outflow from the proto-Planetar
Externí odkaz:
http://arxiv.org/abs/1701.01179
Autor:
Chavez-Dagostino, M., Bertone, E., de Miera, F. Cruz-Saenz, Marshall, J. P., Wilson, G. W., Sanchez-Argüelles, D., Hughes, D. H., Kennedy, G., Vega, O., De la Luz, V., Dent, W. R. F., Eiroa, C., Gomez-Ruiz, A. I., Greaves, J. S., Lizano, S., Lopez-Valdivia, R., Mamajek, E., Montaña, A., Olmedo, M., Rodriguez-Montoya, I., Schloerb, F. P., Yun, M. S., Zavala, J. A., Zeballos, M.
Epsilon Eridani is a nearby, young Sun-like star that hosts a ring of cool debris analogous to the solar system's Edgeworth-Kuiper belt. Early observations at (sub-)mm wavelengths gave tentative evidence of the presence of inhomogeneities in the ring
Externí odkaz:
http://arxiv.org/abs/1606.02761
Autor:
Rojas-García, O S, Gómez-Ruiz, A I, Palau, A, Orozco-Aguilera, M T, Kurtz, S E, Chavez Dagostino, M
Publikováno v:
Monthly Notices of the Royal Astronomical Society; 1/15/2024, Vol. 527 Issue 2, p2110-2127, 18p
Akademický článek
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Autor:
Bruno M., Dagostino M., Morelli L., Gulminelli F., Baiocco G., Barlini S., Casini G., Gramegna F., Kravchuk V. L., Marchi T., Raduta Ad. R.
Publikováno v:
EPJ Web of Conferences, Vol 31, p 00042 (2012)
Odd-even effects in fragment production have been studied since a long time and never quantitatively understood. The odd-even anomaly was reported in the literature [1,2] to be more pronounced in reactions involving Ni projectile and targets, in part
Externí odkaz:
https://doaj.org/article/e8e8a58e8b8b45c29a98bf2f7d9aeb6a
Autor:
MORELLI, L.1, DAGOSTINO, M.1, BRUNO, M.1, GULMINELLI, F.2, BAIOCCO, G.1, BARLINI, S.3, CASINI, G.3, GRAMEGNA, F.4, KRAVCHUK, V. L.4, MARCHI, T.4, RADUTA, AD. R.5
Publikováno v:
EPJ Web of Conferences. 2012, Issue 31, p00042-p.1-00042-p.4. 4p.