1.8k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- University of CataniaIT433 papers
- Centre National de la Recherche ScientifiqueFR334 papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR297 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di CataniaIT243 papers
- Istituto Nazionale di Fisica NucleareIT224 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di NapoliIT203 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di GenovaIT186 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR177 papers
- Sapienza University of RomeIT176 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di BolognaIT173 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di Roma IIT169 papers
- University of GenoaIT168 papers
5 papers · 2 filters
Direct observation of the radial magnetic field gradient in HD58260 from spectropolarimetry of NLTE lines in emission
Marina Giarrusso
Because of the unquestionable presence of magnetic fields in stars, their role in the structure of stellar atmospheres has for a long time been a subject of speculation. In our con…
Presolar grain isotopic ratios as constraints to nuclear and stellar parameters of AGB nucleosynthesis
Sara Palmerini, Maurizio Busso, Diego Vescovi +8
Recent models for evolved Low Mass Stars (with ), undergoing the AGB phase assume that magnetic flux-tube buoyancy drives the formation of C reservoirs…
A scaling relationship for non-thermal radio emission from ordered magnetospheres: from the top of the Main Sequence to planets
P. Leto, C. Trigilio, J. Krticka +20
In this paper, we present the analysis of incoherent non-thermal radio emission from a sample of hot magnetic stars, ranging from early-B to early-A spectral type. Spanning a wide…
Theoretical predictions of surface light element abundances in protostellar and pre-Main Sequence phase
E. Tognelli, S. Degl'Innocenti, P. G. Prada Moroni +5
Theoretical prediction of surface stellar abundances of light elements -- lithium, beryllium, and boron -- represents one of the most interesting open problems in astrophysics. As…
The impact of the new measurement of the fusion cross section on the final compactness of the massive stars
Alessandro Chieffi, Lorenzo Roberti, Marco Limongi +6
We discuss how the new measurement of the fusion cross section carried out with the Trojan Horse Method (Tumino, A., Spitaleri, C., La Cognata, M., et al., 2018, Na…