Zobrazeno 1 - 10
of 931
pro vyhledávání: '"Santamaría E"'
Autor:
Santamaría, E., Toalá, J. A., Liimets, T., Guerrero, M. A., Botello, M. K., Sabin, L., Ramos-Larios, G.
We present an analysis of high-dispersion spectroscopic observations of the symbiotic system R Aquarii (R Aqr) obtained with the Manchester Echelle Spectrograph (MES) at the 2.1 m telescope of the San Pedro M\'artir Observatory (Mexico). An interpret
Externí odkaz:
http://arxiv.org/abs/2404.17710
Publikováno v:
Journal of Asthma and Allergy, Vol Volume 11, Pp 225-231 (2018)
Eva Santamaría,1,2 Iñaki Izquierdo,2 Marta Valle,1,3 Jan Vermeulen,4 Paul Potter5 1Department of Pharmacology, Therapeutics and Toxicology, Universitat Autònoma de Barcelona, Barcelona, Spain; 2Clinical Development, R&D, J. Uriach y Compañía, S.
Externí odkaz:
https://doaj.org/article/e8eb5bb2a7294d1b8ed5d91e56c2f158
We present the analysis of archival Very Large Telescope (VLT) MUSE and multi-epoch Hubble Space Telescope (HST) WFPC2 and WFC3/UVIS narrow-band observations of the remnant associated with the ejecta of the mid-nineteenth century outburst of the recu
Externí odkaz:
http://arxiv.org/abs/2402.07879
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
We present GTC MEGARA high-dispersion integral field spectroscopic observations of the nova remnant QU\,Vul, which provide a comprehensive 3D view of this nova shell. The tomographic analysis of the H$\alpha$ emission reveals a complex physical struc
Externí odkaz:
http://arxiv.org/abs/2209.13722
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
We present long-slit intermediate-dispersion spectroscopic observations and narrow-band direct imaging of four classical nova shells, namely TAur, HRDel, DQHer and QUVul, and the nova-like source CKVul. These are used to construct models of their neb
Externí odkaz:
http://arxiv.org/abs/2202.13946
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:
Rechy-García, J. S., Guerrero, M. A., Santamaría, E., Gómez-González, V. M. A., Ramos-Larios, G., Toalá, J. A., Cazzoli, S., Sabin, L., Miranda, L. F., Fang, X., Liu, J.
HuBi 1 has been proposed to be member of the rare class of born-again planetary nebulae (PNe), i.e., its central star experienced a very late thermal pulse and ejected highly-processed material at high speeds inside the old hydrogen-rich PN. In this
Externí odkaz:
http://arxiv.org/abs/2009.13575
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