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20182026
most citedThe Type II-P Supernova 2017eaw: from explosion to the nebular phase

86 citations · 288 across the 22 of their papers we have counts for

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Showing astro-ph.SRShow all

26 papers · 1 filter

astro-ph.SR2026

Interferometric Images of the Starspot Evolution of Andromedae

Rachael M. Roettenbacher, John D. Monnier, Heidi Korhonen +21

The evolution of starspots of the giant primaries of RS CVn systems is typically detected indirectly with photometric and spectroscopic monitoring. These observations suggest slowl…

astro-ph.SR2026

Stellar Interpretation of Meteoritic Data and PLotting for Everyone (SIMPLE): Isotope Mixing Lines for Six Sets of Core-Collapse Supernova Models

Marco Pignatari, Mattias Ek, Georgy V. Makhatadze +15

Bulk meteorites and their inclusions exhibit, for many chemical elements, isotopic variability produced by nucleosynthetic events in stars and supernovae before the formation of th…

astro-ph.SR2025

The Gothard Observatory Synthetic Stellar Photometry Database

József Kovács, Szabolcs Mészáros, Beáta Harmati +6

Context. In order to determine stellar luminosities and radii, it is necessary to know the total bolometric fluxes emitted by the stars, or equivalently the bolometric corrections…

astro-ph.SR2025

Predictions from -process AGB models of the isotopic variations of zirconium and neodymium for comparison to bulk meteorites

Maria Lugaro, Giulia C. Cinquegrana, Balázs Szányi +6

Bulk meteoritic data show isotopic variability of -neutron-capture (-process) origin in a several elements heavier than Fe. One peculiar feature is that the lighter -pr…

astro-ph.SR20254 cited

Rare Find: Discovery and chemo-dynamical properties of two s-process enhanced RR Lyrae stars

Valentina D'Orazi, Giuliano Iorio, Borbála Cseh +15

We report the serendipitous discovery of two RR Lyrae stars exhibiting significant s-process element enrichment, a rare class previously represented solely by TY Gruis. Our goal is…

astro-ph.SR20254 cited

Short- and long-term variations of the high mass accretion rate classical T Tauri star DR Tau

Gabriella Zsidi, Ágnes Kóspál, Péter Ábrahám +20

Classical T Tauri stars are newly formed, low mass stars which may display both periodic and random variations in their brightness. The interaction between the star and its circums…