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7Be detection in the 2021 outburst of RS Oph

Autor: Molaro, P, Izzo, L, Selvelli, P, Bonifacio, P, Aydi, E, Cescutti, G, Guido, E, J Harvey, E, Hernanz, M, Della , M, Valle

Publikováno v: Molaro, P, Izzo, L, Selvelli, P, Bonifacio, P, Aydi, E, Cescutti, G, Guido, E, Harvey, E J, Hernanz, M & Della Valle, M 2022, ' 7 Be detection in the 2021 outburst of RS Oph ', Monthly Notices of the Royal Astronomical Society, vol. 518, no. 2, pp. 2614-2626 . https://doi.org/10.1093/mnras/stac2708

The recurrent nova RS Oph underwent a new outburst on August 8, 2021, reaching a visible brightness of V = 4.8 mag. Observations of the 2021 outburst made with the high resolution UVES spectrograph at the Kueyen-UT2 telescope of ESO-VLT in Paranal en

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::637cb6b53e5321788b3355eace56669f
https://doi.org/10.1093/mnras/stac2708

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Akademický článek

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Proton acceleration in thermonuclear nova explosions revealed by gamma rays

Autor: MAGIC Collaboration, Acciari, V. A., Ansoldi, S., Antonelli, L. A., Engels, A. Arbet, Artero, M., Asano, K., Baack, D., Babić, A., Baquero, A., de Almeida, U. Barres, Barrio, J. A., Batković, I., González, J. Becerra, Bednarek, W., Bellizzi, L., Bernardini, E., Bernardos, M., Berti, A., Besenrieder, J., Bhattacharyya, W., Bigongiari, C., Biland, A., Blanch, O., Bökenkamp, H., Bonnoli, G., Bošnjak, Ž., Busetto, G., Carosi, R., Ceribella, G., Cerruti, M., Chai, Y., Chilingarian, A., Cikota, S., Colak, S. M., Colombo, E., Contreras, J. L., Cortina, J., Covino, S., D'Amico, G., D'Elia, V., Da Vela, P., Dazzi, F., De Angelis, A., De Lotto, B., Del Popolo, A., Delfino, M., Delgado, J., Mendez, C. Delgado, Depaoli, D., Di Pierro, F., Di Venere, L., Espiñeira, E. Do Souto, Prester, D. Dominis, Donini, A., Dorner, D., Doro, M., Elsaesser, D., Ramazani, V. Fallah, Alonso, L. Fariña, Fattorini, A., Fonseca, M. V., Font, L., Fruck, C., Fukami, S., Fukazawa, Y., López, R. J. García, Garczarczyk, M., Gasparyan, S., Gaug, M., Giglietto, N., Giordano, F., Gliwny, P., Godinović, N., Green, J. G., Green, D., Hadasch, D., Hahn, A., Hassan, T., Heckmann, L., Herrera, J., Hoang, J., Hrupec, D., Hütten, M., Inada, T., Ishio, K., Iwamura, Y., Martínez, I. Jiménez, Jormanainen, J., Jouvin, L., Kerszberg, D., Kobayashi, Y., Kubo, H., Kushida, J., Lamastra, A., Lelas, D., Leone, F., Lindfors, E., Linhoff, L., Lombardi, S., Longo, F., López-Coto, R., López-Moya, M., López-Oramas, A., Loporchio, S., Fraga, B. Machado de Oliveira, Maggio, C., Majumdar, P., Makariev, M., Mallamaci, M., Maneva, G., Manganaro, M., Mannheim, K., Maraschi, L., Mariotti, M., Martínez, M., Aguilar, A. Mas, Mazin, D., Menchiari, S., Mender, S., Mićanović, S., Miceli, D., Miener, T., Miranda, J. M., Mirzoyan, R., Molina, E., Moralejo, A., Morcuende, D., Moreno, V., Moretti, E., Nakamori, T., Nava, L., Neustroev, V., Rosillo, M. Nievas, Nigro, C., Nilsson, K., Nishijima, K., Noda, K., Nozaki, S., Ohtani, Y., Oka, T., Otero-Santos, J., Paiano, S., Palatiello, M., Paneque, D., Paoletti, R., Paredes, J. M., Pavletić, L., Peñil, P., Persic, M., Pihet, M., Moroni, P. G. Prada, Prandini, E., Priyadarshi, C., Puljak, I., Rhode, W., Ribó, M., Rico, J., Righi, C., Rugliancich, A., Sahakyan, N., Saito, T., Sakurai, S., Satalecka, K., Saturni, F. G., Schleicher, B., Schmidt, K., Schweizer, T., Sitarek, J., Šnidarić, I., Sobczynska, D., Spolon, A., Stamerra, A., Strišković, J., Strom, D., Strzys, M., Suda, Y., Surić, T., Takahashi, M., Takeishi, R., Tavecchio, F., Temnikov, P., Terzić, T., Teshima, M., Tosti, L., Truzzi, S., Tutone, A., Ubach, S., van Scherpenberg, J., Vanzo, G., Acosta, M. Vazquez, Ventura, S., Verguilov, V., Vigorito, C. F., Vitale, V., Vovk, I., Will, M., Wunderlich, C., Yamamoto, T., Zarić, D., Ambrosino, F., Cecconi, M., Catanzaro, G., Ferrara, C., Frasca, A., Munari, M., Giustolisi, L., Alonso-Santiago, J., Giarrusso, M., Munari, U., Valisa, P.

Publikováno v: E-Prints Complutense. Archivo Institucional de la UCM
Universidad Europea (UEM)
Nature Astronomy
Digital.CSIC. Repositorio Institucional del CSIC
instname

Acciari, V. A., et al (MAGIC Collaboration). Este artículo tiene una corrección 2022NatAs...6..760A.
Classical novae are cataclysmic binary star systems in which the matter of a companion star is accreted on a white dwarf. Accumulation of hydr

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ee006409acc104f00e2f9b743c0d85b1
http://hdl.handle.net/11577/3455420

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The 2021 outburst of the recurrent nova RS Ophiuchi observed in X-rays by the Neil Gehrels Swift Observatory: a comparative study

Autor: K L Page, A P Beardmore, J P Osborne, U Munari, J-U Ness, P A Evans, M F Bode, M J Darnley, J J Drake, N P M Kuin, T J O’Brien, M Orio, S N Shore, S Starrfield, C E Woodward

Publikováno v: Page, K L, Beardmore, A P, Osborne, J P, Munari, U, Ness, J-U, Evans, P A, {Bode}, M F, Darnley, M J, Drake, J J, Kuin, N P M, O'Brien, T J, Orio, M, Shore, S N, Starrfield, S & Woodward, C E 2022, ' The 2021 outburst of the recurrent nova RS Ophiuchi observed in X-rays by the Neil Gehrels Swift Observatory: a comparative study ', Monthly Notices of the Royal Astronomical Society, vol. 514, no. 2, stac1295, pp. 1557-1574 . https://doi.org/10.1093/mnras/stac1295

On 2021 August 8, the recurrent nova RS Ophiuchi erupted again, after an interval of 15.5 yr. Regular monitoring by the Neil Gehrels Swift Observatory began promptly, on August 9.9 (0.37 day after the optical peak), and continued until the source pas

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::70bbb43ea392d1f41ad5784d86badcb2
http://arxiv.org/abs/2205.03232

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