collaborators

7 papers

astro-ph.GA2025

The ALMA Survey of 70 μm Dark High-mass Clumps in Early Stages (ASHES). XIII. Core Mass Function, Lifetime, and Growth of Prestellar Cores

Kaho Morii, Patricio Sanhueza, Qizhou Zhang +10

The core mass function (CMF) of prestellar cores is essential for understanding the initial conditions of star and cluster formation. However, the universality of the CMF and its r…

astro-ph.GA2025

Dense Molecular Ring-like structure in gaseous CO depletion region G34.74-0.12

Shuting Lin, Siyi Feng, Fengwei Xu +14

We report the discovery of a dense molecular ring-like structure in a dense (10 cm), cold (pc-scale CO depletion at a factor of 5), and young (10 year) star-forming…

astro-ph.GA2025

Cosmic-ray ionisation rate in low-mass cores: the role of the environment

E. Redaelli, S. Bovino, G. Sabatini +6

Context: Cosmic rays drive several key processes for the chemistry and dynamical evolution of star-forming regions. Their effect is quantified mainly by means of the cosmic-ray ion…

astro-ph.GA2025

The ALMA Survey of 70 m Dark High-mass Clumps in Early Stages (ASHES). XII. Unanchored Forked Stream in the Propagating Path of a Protostellar Outflow

Shuting Lin, Siyi Feng, Patricio Sanhueza +14

Outflows are key indicators of ongoing star formation. We report the discovery of an unanchored forked stream within the propagating path of an extremely young protostellar outflow…

astro-ph.GA2025

Impact of cosmic-ray propagation on the chemistry and ionisation fraction of dark clouds

G. Latrille, A. Lupi, S. Bovino +3

A proper modelling of the cosmic-ray ionisation rate within gas clouds is crucial to describe their chemical evolution accurately. However, this modelling is computationally demand…

astro-ph.SR2025

Gas infall via accretion disk feeding Cepheus A HW2

A. Sanna, A. Oliva, L. Moscadelli +10

The star-forming region Cepheus A hosts a very young star, called HW2, that is the second closest to us growing a dozen times more massive than our Sun. The circumstellar environme…