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researcher

Dorottya Szécsi

5 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author3
  • last author1

Across the 5 of 5 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3
  • astro-ph.GA1
  • astro-ph.HE1
ORCID 0000-0001-6473-7085

identity via Semantic Scholar / OpenAlex

activity
20122024
most citedCommon envelope ejection in massive binary stars - Implications for the progenitors of GW150914 and GW151226

138 citations · 256 across the 5 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2016★ 86 cited

The metallicity dependence of envelope inflation in massive stars

D. Sanyal, N. Langer, D. Szécsi +2

Recently it has been found that models of massive stars reach the Eddington limit in their interior, which leads to dilute extended envelopes. We perform a comparative study of the…

astro-ph.SR2016★ 138 cited

Common envelope ejection in massive binary stars - Implications for the progenitors of GW150914 and GW151226

M. U. Kruckow, T. M. Tauris, N. Langer +3

The recently detected gravitational wave signals (GW150914 and GW151226) of the merger event of a pair of relatively massive stellar-mass black holes (BHs) calls for an investigati…

astro-ph.HE2012

GRB duration distribution considering the position of the Fermi

Dorottya Szecsi, Zsolt Bagoly, Istvan Horvath +3

The Fermi satellite has a particular motion during its flight which enables it to catch the gamma-ray bursts mostly well. The side-effect of this favourable feature is that the lig…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.