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pro vyhledávání: '"Molina B"'
Autor:
Tateo A, Siquier-Dameto G, Artzi O, Humzah D, Molina B, Jain R, Lanzarotti A, Laouedj M, Dapis N, Bellia G
Publikováno v:
Clinical, Cosmetic and Investigational Dermatology, Vol Volume 14, Pp 349-354 (2021)
Antonello Tateo,1 Gabriel Siquier-Dameto,2– 4 Ofir Artzi,5 Dalvi Humzah,6 Beatriz Molina,7 Ravi Jain,6 Arturo Lanzarotti,8 Malika Laouedj,9 Nicolas Dapis,10 Gilberto Bellia11 1Private Practice, Milan, Italy; 2Private Practice, Amsterdam, the Nether
Externí odkaz:
https://doaj.org/article/3ef75879f5ca4deba7df5e8c6ce72330
We present the analysis of spatially-resolved spectroscopic observations of the born-again planetary nebula (PN) A 78 that are used to investigate the chemistry and physical properties of its three main morphological components, namely the inner knot
Externí odkaz:
http://arxiv.org/abs/2309.08242
Autor:
Sokolovsky, K. V., Johnson, T. J., Buson, S., Jean, P., Cheung, C. C., Mukai, K., Chomiuk, L., Aydi, E., Molina, B., Kawash, A., Linford, J. D., Mioduszewski, A. J., Rupen, M. P., Sokoloski, J. L., Williams, M. N., Steinberg, E., Vurm, I., Metzger, B. D., Page, K. L., Orio, M., Quimby, R. M., Shafter, A. W., Corbett, H., Bolzoni, S., DeYoung, J., Menzies, K., Romanov, F. D., Richmond, M., Ulowetz, J., Vanmunster, T., Williamson, G., Lane, D. J., Bartnik, M., Bellaver, M., Bruinsma, E., Dugan, E., Fedewa, J., Gerhard, C., Painter, S., Peterson, D. -M., Rodriguez, J. E., Smith, C., Sullivan, H., Watson, S.
Classical novae are shock-powered multi-wavelength transients triggered by a thermonuclear runaway on an accreting white dwarf. V1674 Her is the fastest nova ever recorded (time to declined by two magnitudes is t_2=1.1 d) that challenges our understa
Externí odkaz:
http://arxiv.org/abs/2302.03043
Autor:
Rodríguez-González, J. B., Santamaría, E., Toalá, J. A., Guerrero, M. A., Montoro-Molina, B., Rubio, G., Tafoya, D., Chu, Y. -H., Ramos-Larios, G., Sabin, L.
Born-again planetary nebulae (PNe) are extremely rare cases in the evolution of solar-like stars. It is commonly accepted that their central stars (CSPN) experienced a very late thermal pulse (VLTP), ejecting H-deficient material inside the evolved H
Externí odkaz:
http://arxiv.org/abs/2204.08501
Autor:
Montoro-Molina, B., Guerrero, M. A., Pérez-Díaz, B., Toalá, J. A., Cazzoli, S., Bertolami, M. M. Miller, Morisset, C.
The central star of the planetary nebula (PN) HuBi\,1 has been recently proposed to have experienced a very late thermal pulse (VLTP), but the dilution of the emission of the recent ejecta by that of the surrounding H-rich old outer shell has so far
Externí odkaz:
http://arxiv.org/abs/2202.00353
We present the first 3D radiation-hydrodynamic simulations on the formation and evolution of born-again planetary nebulae (PNe), with particular emphasis to the case of HuBi1, the inside-out PN. We use the extensively-tested GUACHO code to simulate t
Externí odkaz:
http://arxiv.org/abs/2103.11503
Autor:
Guerrero, M. A., Cazzoli, S., Rechy-Garcia, J. S., Ramos-Larios, G., Montoro-Molina, B., Gomez-Gonzalez, V. M. A., Toala, J. A., Fang, X.
Jets (fast collimated outflows) are claimed to be the main shaping agent of the most asymmetric planetary nebula (PNe) as they impinge on the circumstellar material at late stages of the asymptotic giant branch (AGB) phase. The first jet detected in
Externí odkaz:
http://arxiv.org/abs/2102.01093
Akademický článek
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Autor:
Gaget, E.1 lie.gaget@gmail.com, Galewski, T.2, Brommer, J. E.1, Le Viol, I.3,4, Jiguet, F.3, Baccetti, N.5, Langendoen, T.6, Molina, B.7, Moniz, F.8, Moussy, C.9, Zenatello, M.5, Guillemain, M.10
Publikováno v:
Animal Conservation. Feb2024, Vol. 27 Issue 1, p5-16. 12p.