activity
20242026
collaborators

7 papers

astro-ph.GA2026

A new hot core in the outer Galaxy: Impact of metallicity on the formation of complex organic molecules

Youxin Wang, Arnaud Belloche, Robin T. Garrod

Many complex organic molecules (COMs) in star-forming regions are believed to form on dust grains. We thus expect both the reduced metallicity and dust-to-gas ratio in the outer Ga…

astro-ph.GA2025

Hunting pre-stellar cores with APEX: overview

P. Caselli, S. Spezzano, E. Redaelli +8

[Abridged] Pre-stellar cores are centrally concentrated starless cores on the verge of star formation and they represent the initial conditions for star and planet forma…

astro-ph.GA2025

Statistical nuclear spin ratios of deuterated ammonia in the pre-stellar core L1544

Jorma Harju, Paola Caselli, Olli Sipilae +6

We determined the ortho/para (o/p) ratios of NH2D and NHD2 in the archetypical pre-stellar core L1544. The core was observed in the two lowest rotational lines of ortho- and para-N…

astro-ph.GA2025

Reexploring Molecular Complexity with ALMA: Insights into chemical differentiation from the molecular composition of hot cores in Sgr B2(N2)

A. Belloche, R. T. Garrod, H. S. P. Müller +3

We used ALMA to perform a line survey of the high-mass star forming region Sgr B2(N), called ReMoCA. We modeled under the assumption of LTE the spectra obtained toward the sources…

astro-ph.SR2025

Hunting pre-stellar cores with APEX: Corona Australis 151, the densest pre-stellar core or the youngest protostar?

E. Redaelli, S. Spezzano, P. Caselli +6

Context. Pre-stellar cores are the birthplaces of Sun-like stars and represent the initial conditions for the assembly of protoplanetary systems. Due to their short lifespans, they…

astro-ph.SR2025

Molecular inventory of a young eruptive star's environment -- Case study of the classical FU Orionis star V1057 Cyg

Zs. M. Szabó, A. Belloche, K. M. Menten +6

Studying accretion-driven episodic outbursts in YSOs is key to understanding the later stages of star and planet formation. FU Orionis-type objects form a YSO subclass, distinguish…