Zobrazeno 1 - 10
of 2 449
pro vyhledávání: '"Rubio, G"'
Theory predicts that the temperature of the X-ray-emitting gas ($\sim$10$^{6}$ K) detected from planetary nebulae (PNe) is a consequence of mixing or thermal conduction when in contact with the ionized outer rim ($\sim$10$^{4}$ K). Gas at intermediat
Externí odkaz:
http://arxiv.org/abs/2210.09116
Autor:
Ferrer, E., Rubio, G., Ntoukas, G., Laskowski, W., Mariño, O. A., Colombo, S., Mateo-Gabín, A., de Lara, F. Manrique, Huergo, D., Manzanero, J., Rueda-Ramírez, A. M., Kopriva, D. A., Valero, E.
We present the latest developments of our High-Order Spectral Element Solver (HORSES3D), an open source high-order discontinuous Galerkin framework, capable of solving a variety of flow applications, including compressible flows (with or without shoc
Externí odkaz:
http://arxiv.org/abs/2206.09733
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
3D mapping of the Wolf-Rayet nebula M1-67: clues for post-common envelope evolution in massive stars
Autor:
Zavala, S., Toalá, J. A., Santamarí, E., Ramos-Larios, G., Sabin, L., Quino-Mendoza, J. A., Rubio, G., Guerrero, M. A.
We present a 3D mapping of the Wolf-Rayet (WR) nebula M1-67 around WR124. We obtained high-resolution San Pedro M\'{a}rtir (SPM) Manchester Echelle Spectrograph (MES) observations along 17 long-slit positions covering all morphological features in M1
Externí odkaz:
http://arxiv.org/abs/2204.07778
Autor:
Gómez-González, V. M. A., Rubio, G., Toalá, J. A., Guerrero, M. A., Sabin, L., Todt, H., Gómez-Llanos, V., Ramos-Larios, G., Mayya, Y. D.
We present a multi-wavelength characterisation of the planetary nebula (PN) NGC 6905 and its [Wolf-Rayet]-type ([WR]) central star (CSPN) HD 193949. Our Nordic Optical Telescope (NOT) Alhambra Faint Object Spectrograph and Camera (ALFOSC) spectra and
Externí odkaz:
http://arxiv.org/abs/2110.09551
Autor:
Toalá, J. A., Rubio, G., Santamaría, E., Guerrero, M. A., Estrada-Dorado, S., Ramos-Larios, G., Sabin, L.
We present the analysis of XMM-Newton European Photon Imaging Camera (EPIC) observations of the nova shell IPHASX J210204.7$+$471015. We detect X-ray emission from the progenitor binary star with properties that resemble those of underluminous interm
Externí odkaz:
http://arxiv.org/abs/2101.11480
Autor:
Rubio, G., Toalá, J. A., Jiménez-Hernández, P., Ramos-Larios, G., Guerrero, M. A., Gómez-González, V. M. A., Santamaría, E., Quino-Mendoza, J. A.
We present a comprehensive infrared (IR) study of the iconic Wolf-Rayet (WR) wind-blown bubble NGC6888 around WR136. We use Wide-field Infrared Survey Explorer (WISE), Spitzer IRAC and MIPS and Herschel PACS IR images to produce a sharp view of the d
Externí odkaz:
http://arxiv.org/abs/2009.05479
Autor:
Santamaría, E., Guerrero, M. A., Ramos-Larios, G., Toalá, J. A., Sabin, L., Rubio, G., Quino-Mendoza, J. A.
Nova shells can provide us with important information on their distance, their interactions with the circumstellar and interstellar media, and the evolution in morphology of the ejecta. We have obtained narrow-band images of a sample of five nova she
Externí odkaz:
http://arxiv.org/abs/2002.06749
We study a five-dimensional non-relativistic gravity theory whose action is composed of a gravitational sector and a sector of matter where the gravitational sector is given by the so called Newton--Chern--Simons gravity and where the matter sector i
Externí odkaz:
http://arxiv.org/abs/1911.05448
Autor:
Sansores, R.H., Ramírez-Venegas, A., Montiel-Lopez, F., Domínguez-Arellano, S., Alva-Lopez, L.F., Falfán-Valencia, R., Pérez-Rubio, G., Olaya-López, E., Zavaleta-Martínez, E.O., Aguilar-Medina, S., Escobar-Alvarado, J.C., Poo, J.L., Matera, M.G., Cazzola, M.
Publikováno v:
In Respiratory Medicine October 2023 217