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C. Iliadis

4 papers hereh-index 8342 citations18 works total

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

author position
  • sole author1
  • middle author2
  • last author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR2
  • astro-ph.HE1
  • nucl-ex1
same name
  • C. Iliadis — 2 papers, h 13
  • C. Iliadis — 2 papers, h 3

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

collaborators

4 papers

astro-ph.SR2025

Elemental and Isotopic Yields from T Coronae Borealis: Predictions and Uncertainties

Emma Wallace, Christian Iliadis, Sumner Starrfield

T Coronae Borealis (T CrB) is a symbiotic recurrent nova system expected to undergo its next outburst within the next two years. Recent hydrodynamic simulations have predicted the…

astro-ph.HE2025

Low-metallicity nova explosions: a site for weak rp-process nucleosynthesis

Athanasios Psaltis, Jordi José, Richard Longland +1

Classical novae are common cataclysmic events involving a binary system of a white dwarf and a main sequence or red giant companion star. In metal-poor environments, these explosio…

nucl-ex2025

Deciphering Spin-Parity Assignments of Nuclear Levels

Christian Iliadis

Spin-parity assignments of nuclear levels are critical for understanding nuclear structure and reactions. However, inconsistent notation conventions and ambiguous reporting in rese…

astro-ph.SR2025

Hydrodynamic Predictions for the Next Outburst of T Coronae Borealis: It will be the Brightest Classical or Recurrent Nova Ever Observed in X-rays

S. Starrfield, M. Bose, C. E. Woodward +11

T Coronae Borealis (TCrB) is a recurrent nova (RN) with recorded outbursts in 1866, and 1946 and possible outbursts in 1217 and 1787. It is predicted to explode again in 2025 or 20…

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