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Ángel Giménez
Antiguo investigador BC3
Principal línea de investigación:
Ecosystem Services Modeling
Was employee in BC3 from 2019-11-01 to 2021-12-15
Short CV
I am graduated in Mathematics, doctor in Astrophysics and I hold a master's degree in Agro- and Ecosystems Engineering. I've also worked as a software developer.
As a modeler of Ecosystem Services at BC3, I am enthusiastic about using models that help us to better understand nature and, in so doing, promote its conservation.
Affiliation previous to BC3
Giménez-García, A., T. Shenar, J.M. Torrejón, L. Oskinova, S. Martínez-Núñez, W.-R. Hamann, J.J. Rodes-Roca, et al. “Measuring the Stellar Wind Parameters in IGR J17544-2619 and Vela X-1 Constrains the Accretion Physics in Supergiant Fast X-Ray Transient and Classical Supergiant X-Ray Binaries.” Astronomy and Astrophysics 591 (2016).Giménez-García, A., J.M. Torrejón, W. Eikmann, S. Martínez-Núñez, L.M. Oskinova, J.J. Rodes-Roca, and G. Bernabéu. “An XMM-Newton View of FeKalpha In High-Mass X-Ray Binaries.” Astronomy and Astrophysics 576 (2015).
Kretschmar, P., S. Martínez-Núñez, E. Bozzo, L.M. Oskinova, J. Puls, L. Sidoli, J.O. Sundqvist, et al. “Stellar Winds in Massive X-Ray Binaries.” Proceedings of the International Astronomical Union 12, no. S329 (2016): 355–58.
Martínez-Núñez, S., P. Kretschmar, E. Bozzo, L.M. Oskinova, J. Puls, L. Sidoli, J.O. Sundqvist, et al. “Towards a Unified View of Inhomogeneous Stellar Winds in Isolated Supergiant Stars and Supergiant High Mass X-Ray Binaries.” Space Science Reviews 212, no. 1-2 (2017): 59–150.
Martínez-Núñez, S., A. Sander, A. Gímenez-García, A. Gónzalez-Galán, J.M. Torrejón, C. Gónzalez-Fernández, and W.-R. Hamann. “The Donor Star of the X-Ray Pulsar X1908+075.” Astronomy and Astrophysics 578 (2015).
Rodes-Roca, J.J., T. Mihara, S. Nakahira, J.M. Torrejón, ?. Giménez-García, and G. Bernabéu. “Orbital Phase-Resolved Spectroscopy of 4U 1538-52 with MAXI.” Astronomy and Astrophysics 580 (2015).
Rodes-Roca, J.J., J.M. Torrejón, S. Martínez-Nuñez, A. Giménez-García, and G. Bernabéu. “Discussing the Physical Meaning of the Absorption Feature at 2.1 Kev in 4U 1538-52.” Astronomische Nachrichten 335, no. 8 (2014): 804–11.
Sander, A., T. Shenar, R. Hainich, A. Gímenez-García, H. Todt, and W.-R. Hamann. “On the Consistent Treatment of the Quasi-Hydrostatic Layers in Hot Star Atmospheres.” Astronomy and Astrophysics 577 (2015).
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