no code implementations • 24 Feb 2021 • R. Amato, V. Grinberg, N. Hell, S. Bianchi, C. Pinto, D. D'Aí, M. Del Santo, T. Mineo, A. Santangelo
The Supergiant X-ray binary Vela X-1 represents one of the best astrophysical sources to investigate the wind environment of a O/B star irradiated by an accreting neutron star.
High Energy Astrophysical Phenomena
no code implementations • 16 Oct 2020 • P. Chakraborty, G. J. Ferland, S. Bianchi, M. Chatzikos
We update the ionization potential ($I_{\rm ion}$) for these elements and add a fourth-order polynomial to the level energy difference.
Instrumentation and Methods for Astrophysics High Energy Astrophysical Phenomena
1 code implementation • 14 Oct 2019 • W. Dobbels, M. Baes, S. Viaene, S. Bianchi, J. I. Davies, V. Casasola, C. J. R. Clark, J. Fritz, M. Galametz, F. Galliano, A. Mosenkov, A. Nersesian, A. Trčka
This results in a 'virtual FIR telescope', which can be applied to large optical-MIR galaxy samples.
Astrophysics of Galaxies
