activity
20162026
most citedThe Natural History of 'Oumuamua

121 citations · 538 across the 18 of their papers we have counts for

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Showing astro-ph.SRShow all

9 papers · 1 filter

astro-ph.SR2026

Ionized gas emission in protoplanetary disks with the SKAO

Greta Guidi, Christian Rab, Barbara Ercolano +20

Protoplanetary disks represent a crucial stage in the evolution of Young Stellar Objects towards the formation of fully formed planetary systems. While substantial progress has bee…

astro-ph.SR2025★ 4 cited

Turn up the light: Radiative efficiency of protostars at birth

Asmita Bhandare, Adnan Ali Ahmad, Benoît Commerçon

Early stages of stellar birth comprise of a two-step process involving the formation of two hydrostatic cores. The second step of gravitational collapse sets the radiative efficien…

astro-ph.SR2024★ 16 cited

Mixing is easy: New insights for cosmochemical evolution from pre-stellar core collapse

Asmita Bhandare, Benoît Commerçon, Guillaume Laibe +5

Signposts of early planet formation are ubiquitous in substructured young discs. Dense, hot and high-pressure regions formed during gravitational collapse process, integral to star…

astro-ph.SR2023

The Exceptional Ring of buoyancy instability in stars

Armand Leclerc, Lucien Jezequel, Nicolas Perez +3

We reveal properties of global modes of linear buoyancy instability in stars, characterised by the celebrated Schwarzschild criterion, using non-Hermitian topology. We identify a r…

astro-ph.SR2021★ 24 cited

Significant interstellar object production by close stellar flybys

Susanne Pfalzner, Luis Aizpuru Vargas, Asmita Bhandare +1

Within just two years, two interstellar objects (ISOs) - Oumuamuas and Borisov - have been discovered. Large quantities of planetesimals form as a by-product of planet formation. T…

astro-ph.SR2020★ 63 cited

Zooming in on Individual Star Formation: Low- and High-mass Stars

Anna L. Rosen, Stella S. R. Offner, Sarah I. Sadavoy +3

Star formation is a multi-scale, multi-physics problem ranging from the size scale of molecular clouds (10s pc) down to the size scales of dense prestellar cores (0.1 p…

astro-ph.SR2020★ 33 cited

Birth of convective low-mass to high-mass second Larson cores

Asmita Bhandare, Rolf Kuiper, Thomas Henning +3

Stars form as an end product of the gravitational collapse of cold, dense gas in magnetized molecular clouds. This multi-scale scenario occurs via the formation of two quasi-hydros…

astro-ph.SR2020★ 74 cited

Formation and Evolution of Disks around Young Stellar Objects

Bo Zhao, Kengo Tomida, Patrick Hennebelle +9

Recent observations have suggested that circumstellar disks may commonly form around young stellar objects. Although the formation of circumstellar disks can be a natural result of…

astro-ph.SR2018★ 41 cited

First Core Properties: From Low- to High-mass Star Formation

Asmita Bhandare, Rolf Kuiper, Thomas Henning +3

In this study, the main goal is to understand the molecular cloud core collapse through the stages of first and second hydrostatic core formation. We investigate the properties of…