Dorottya Szécsi, Ph.D
Affiliations: | 2012-2016 | Rheinische Friedrich-Wilhelms-Universität Bonn, Bonn, Nordrhein-Westfalen, Germany | |
2016-2017 | Astronomical Institute of the Czech Academy of Sciences | ||
2017- | School of Physics and Astronomy and Institute of Gravitational Wave Astronomy | University of Birmingham, Birmingham, England, United Kingdom |
Website:
http://www.sr.bham.ac.uk/~dszecsi/Google:
"Dorottya Szécsi"
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Publications
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Stevenson S, Sampson M, Powell J, et al. (2019) The Impact of Pair-instability Mass Loss on the Binary Black Hole Mass Distribution The Astrophysical Journal. 882: 121 |
Szécsi D, Wünsch R. (2019) Role of Supergiants in the Formation of Globular Clusters The Astrophysical Journal. 871: 20 |
Neijssel CJ, Vigna-Gómez A, Stevenson S, et al. (2019) The effect of the metallicity-specific star formation history on double compact object mergers Monthly Notices of the Royal Astronomical Society. 490: 3740-3759 |
Kubátová B, Szécsi D, Sander AAC, et al. (2019) Low-metallicity massive single stars with rotation: II. Predicting spectra and spectral classes of chemically homogeneously evolving stars Astronomy and Astrophysics. 623 |
Vigna-Gómez A, Neijssel CJ, Stevenson S, et al. (2018) On the formation history of Galactic double neutron stars Monthly Notices of the Royal Astronomical Society. 481: 4009-4029 |
Szécsi D, Mackey J, Langer N. (2018) Supergiants and their shells in young globular clusters Astronomy and Astrophysics. 612 |
Stratta G, Ciolfi R, Amati L, et al. (2018) THESEUS: A key space mission concept for Multi-Messenger Astrophysics Advances in Space Research. 62: 662-682 |
Amati L, O’Brien P, Götz D, et al. (2018) The THESEUS space mission concept: science case, design and expected performances Advances in Space Research. 62: 191-244 |
Sanyal D, Langer N, Szécsi D, et al. (2017) Metallicity dependence of envelope inflation in massive stars Astronomy and Astrophysics. 597 |
Kruckow MU, Tauris TM, Langer N, et al. (2016) Common-envelope ejection in massive binary stars - Implications for the progenitors of GW150914 and GW151226 Astronomy and Astrophysics. 596 |