activity
20142023
most citedDust absorption and scattering in the silicon K-edge

43 citations · 167 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2023★ 32 cited

The -process nucleosynthesis in core-collapse supernovae. I. A novel analysis of -process yields in massive stars

L. Roberti, M. Pignatari, A. Psaltis +4

The -process nucleosynthesis in core-collapse supernovae is generally accepted as a feasible process for the synthesis of neutron-deficient isotopes beyond iron. However, crucia…

nucl-ex2023★ 9 cited

Cross Section Measurement of the Kr(p,)Rb Reaction in Inverse Kinematics

A. Tsantiri, A. Palmisano-Kyle, A. Spyrou +16

The total cross section of the Kr(p,)Rb reaction was measured for the first time at effective center-of-mass energies between 2.4 and 3.0 MeV, within the relevant…

nucl-ex2023★ 10 cited

Cross section measurement of the 144Sm(alpha,n)147Gd reaction for studying the alpha-nucleus optical potential at astrophysical energies

Gy. Gyürky, P. Mohr, A. Angyal +6

Nuclear reactions involving alpha particles play an important role in various astrophysical processes such as the gamma-process of heavy element nucleosynthesis. The poorly known l…

nucl-ex2022★ 12 cited

Study of the Mg waiting point relevant for x-ray burst nucleosynthesis via the Mg(,)Al reaction

H. Jayatissa, M. L. Avila, K. E. Rehm +13

The Mg(,)Al reaction rate has been identified as a major source of uncertainty for understanding the nucleosynthesis flow in Type-I x-ray bursts (XRBs). We repo…

astro-ph.HE2022★ 33 cited

Constraining nucleosynthesis in neutrino-driven winds: observations, simulations and nuclear physics

A. Psaltis, A. Arcones, F. Montes +4

A promising astrophysical site to produce the lighter heavy elements of the first -process peak () is the moderately neutron rich () neutrino-driven…

nucl-ex2022★ 10 cited

First direct measurement of the N(,)O reaction relevant for core-collapse supernovae nucleosynthesis

H. Jayatissa, M. L. Avila, K. E. Rehm +10

Understanding the explosion mechanism of a core-collapse supernova (CCSN) is important to accurately model CCSN scenarios for different progenitor stars using model-observation com…

astro-ph.GA2021★ 11 cited

The Fe(n, γ)Fe Cross Section from the Surrogate Ratio Method and Its Effect on the Fe Nucleosynthesis

S. Q. Yan, X. Y. Li, K. Nishio +39

The long-lived Fe (with a half-life of 2.62 Myr) is a crucial diagnostic of active nucleosynthesis in the Milky Way galaxy and in supernovae near the solar system. The neutr…

astro-ph.GA2019★ 43 cited

Dust absorption and scattering in the silicon K-edge

S. T. Zeegers, E. Costantini, D. Rogantini +5

The composition and properties of interstellar silicate dust are not well understood. In X-rays, interstellar dust can be studied in detail by making use of the fine structure feat…

astro-ph.EP2014★ 7 cited

Absorption of crystalline water ice in the far infrared at different temperatures

Caroline Reinert, Harald Mutschke, Alexander Krivov +2

The optical properties of ice in the far infrared are important for models of protoplanetary and debris disks. In this report we derive a new set of data for the absorption (repres…