activity
20182026
most citedDiscovery of a sub-Keplerian disk with jet around a 20Msun young star. ALMA observations of G023.01-00.41

65 citations · 221 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2026

Formation and X-ray emission from hot bubbles in planetary nebulae - III. The impact of [Wolf-Rayet]-type winds

Rogelio Orozco-Duarte, Jesús A. Toalá, S. Jane Arthur +3

We use radiation-hydrodynamical simulations to investigate the formation and synthetic X-ray emission of hot bubbles within planetary nebulae (PNe) driven by the powerful winds of…

astro-ph.SR2025

Testing the bloated star hypothesis in the massive young stellar object IRAS 19520+2759 through optical and infrared variability

Rakesh Pandey, Aina Palau, Javier Serna +8

Using optical time series with Telescopi Joan Oró (TJO), Gaia, TESS, and NEOWISE archival data, we performed a variability study on the candidate bloated massive young stellar obje…

astro-ph.SR2024★ 7 cited

The Role of Thermal Instability in Accretion Outbursts in High-Mass Stars

Vardan G. Elbakyan, Sergei Nayakshin, Alessio Caratti o Garatti +2

High-mass young stellar objects (HMYSOs) can exhibit episodic bursts of accretion, accompanied by intense outflows and luminosity variations. Thermal Instability (TI) due to Hydrog…

astro-ph.SR2024★ 4 cited

The High-resolution Accretion Disks of Embedded protoStars (HADES) simulations. I. Impact of Protostellar Magnetic Fields on the Accretion Modes

Brandt A. L. Gaches, Jonathan C. Tan, Anna L. Rosen +1

How embedded, actively accreting low-mass protostars accrete their mass is still greatly debated. Observations are now piecing together the puzzle of embedded protostellar accretio…

astro-ph.HE2024

Radiation hydrodynamical simulations of super-Eddington mass transfer and black hole growth in close binaries

Daisuke Toyouchi, Kenta Hotokezaka, Kohei Inayoshi +1

Radiation-driven outflows play a crucial role in extracting mass and angular momentum from binary systems undergoing rapid mass transfer at super-Eddington rates. To study the mass…

astro-ph.SR2023★ 6 cited

A probable Keplerian disk feeding an optically revealed massive young star

Anna F. McLeod, Pamela D. Klaassen, Megan Reiter +3

The canonical picture of star formation involves disk-mediated accretion, with Keplerian accretion disks and associated bipolar jets primarily observed in nearby, low-mass young st…