Zobrazeno 1 - 9
of 9
pro vyhledávání: '"R. G. Izzard"'
Autor:
Nina S Sartorio, A Fialkov, T Hartwig, G M Mirouh, R G Izzard, M Magg, R S Klessen, S C O Glover, L Chen, Y Tarumi, D D Hendriks
The first population of X-ray binaries (XRBs) is expected to affect the thermal and ionization states of the gas in the early Universe. Although these X-ray sources are predicted to have important implications for high-redshift observable signals, su
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c0cc384ccd691420171211cdf5130e1d
Autor:
D. D. Hendriks, R. G. Izzard
Publikováno v:
Journal of Open Source Software. 8:4642
We present the software package binary_c-python which provides a convenient and easy-to-use interface to the binary_c framework, allowing the user to rapidly evolve individual systems and populations of stars. binary_c-python is available on Pip and
In the single-degenerate scenario of Type Ia supernovae (SNe Ia), the interaction between high-speed ejected material and the donor star in a binary system is expected to lead to mass being stripped from the donor. A series of multi-dimensional hydro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ea4761dc7311ab461063ab32dd79d276
http://arxiv.org/abs/2205.09917
http://arxiv.org/abs/2205.09917
Autor:
T Gessey-Jones, N S Sartorio, A Fialkov, G M Mirouh, M Magg, R G Izzard, E de Lera Acedo, W J Handley, R Barkana
Properties of the first generation of stars [referred to as the Population III (Pop III) stars], such as their initial mass function (IMF), are poorly constrained by observations and have yet to converge between simulations. The cosmological 21-cm si
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::28bfaf4f173aeb70a4ccad23d39939ab
http://arxiv.org/abs/2202.02099
http://arxiv.org/abs/2202.02099
Publikováno v:
Astronomy & Astrophysics
Publikováno v:
AIP Conference Proceedings.
We show the preliminary results of our search for the progenitor systems of type Ia supernovae (SNe Ia). We model binary populations our aim being to compare these models with the observations of detailed element abundances of the hot Intra‐Cluster
Autor:
F. R. N. Schneider, O. H. Ramírez-Agudelo, F. Tramper, J. M. Bestenlehner, N. Castro, H. Sana, C. J. Evans, C. Sabín-Sanjulián, S. Simón-Díaz, N. Langer, L. Fossati, G. Gräfener, P. A. Crowther, S. E. de Mink, A. de Koter, M. Gieles, A. Herrero, R. G. Izzard, V. Kalari, R. S. Klessen, D. J. Lennon, L. Mahy, J. Maíz Apellániz, N. Markova, J. Th. van Loon, J. S. Vink, N. R. Walborn
Publikováno v:
Astronomy & Astrophysics
Autor:
E. Zapartas, S. E. De Mink, S. D. Van Dyk, O. D. Fox, N. Smith, K. A. Bostroem, A. De Koter, A. V. Filippenko, R. G. Izzard, P. L. Kelly, C. J. Neijssel, M. Renzo, S. Ryder
Publikováno v:
Astrophysical Journal; 6/20/2017, Vol. 842 Issue 2, p1-1, 1p
Publikováno v:
Astrophysical Journal; 5/20/2015, Vol. 805 Issue 1, p1-1, 1p