activity
20172026
most citedThe observed chemical structure of L1544

87 citations · 278 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.SR2026

Chemical Complexity in the Early Stages of Star Formation in the SKAO Era

Eleonora Bianchi, Mathilde Bouvier, Claudio Codella +44

About 350 molecules have been identified in the interstellar medium (ISM), including complex molecules relevant to prebiotic chemistry. A remarkable level of molecular diversity ha…

astro-ph.GA2026

Jets and Outflows in Young Stellar Objects with the SKAO

Giovanni Sabatini, Gemma Busquet, Carlos Carrasco-González +48

Jets and outflows are ubiquitous phenomena associated with the formation of young stellar objects (YSOs). They play a crucial role in removing angular momentum from the accreting s…

astro-ph.GA2025

Laboratory Detection and Rotational Spectroscopy of -HNSO: Implications for Astronomical Observations

Valerio Lattanzi, Miguel Sanz-Novo, Víctor M. Rivilla +2

Sulfur-bearing molecules are central to interstellar chemistry, yet their observed abundances in the gas phase remain far below cosmic expectations in dense interstellar regions. M…

astro-ph.GA2025★ 4 cited

A detection of sulfur-bearing cyclic hydrocarbons in space

Mitsunori Araki, Miguel Sanz-Novo, Christian P. Endres +13

Molecules harbouring sulfur are thought to have played a key role in the biological processes of life on Earth, and thus, they are of much interest when found in space. Here we rep…

astro-ph.GA2025★ 6 cited

Resolved Gas Temperatures and 12C/13C ratios in SVS13A from ALMA Observations of CH3CN and CH3-13-CN

T. -H. Hsieh, J. E. Pineda, D. M. Segura-Cox +11

Context. Multiple systems are common in field stars, and the frequency is found to be higher in early evolutionary stages. Thus, the study of young multiple systems during the embe…

astro-ph.GA2025★ 31 cited

On the abiotic origin of dimethyl sulfide: discovery of DMS in the Interstellar Medium

Miguel Sanz-Novo, Víctor M. Rivilla, Christian P. Endres +14

Following the discovery of dimethyl sulfide (CHSCH, DMS) signatures in comet 67P/Churyumov-Gerasimenko, we report the first detection of this organosulfur species in the in…

astro-ph.GA2025

Laboratory rotational spectroscopy leads to the first interstellar detection of singly deuterated methyl mercaptan (CHDSH)

Hayley A. Bunn, Silvia Spezzano, Laurent H. Coudert +8

We report an extensive rotational spectroscopic analysis of singly deuterated methyl mercaptan (CHDSH) using both millimeter and far-infrared synchrotron spectra to achieve a…

astro-ph.GA2024★ 4 cited

Advancing spectroscopic understanding of HOCS: Laboratory investigations and astronomical implications

Valerio Lattanzi, Miguel Sanz-Novo, Víctor M. Rivilla +5

Sulphur-bearing species play crucial roles in interstellar chemistry, yet their precise characterisation remains challenging. Here, we present laboratory experiments aimed at exten…

astro-ph.GA2024

Millimeter and submillimeter spectroscopy of the deuterated molecular ion SD+

Mitsunori Araki, Valerio Lattanzi, Christian P. Endres +1

Seven rotational and fine-structure transitions of the deuterated molecular ion SD+ in the X 3S- ground electronic state have been measured in the 271-863 GHz region in the laborat…

astro-ph.GA2024

Accurate ab initio spectroscopic studies of promising interstellar ethanolamine iminic precursors

D. Alberton, N. Inostroza-Pino, Ryan C. Fortenberry +4

Context. The detection of NH2CH2CH2OH (ethanolamine) in molecular cloud G+0.693-0.027 adds an additional player to the prebiotic molecules discovered so far in the interstellar med…

astro-ph.IM2023★ 4 cited

Rotational spectroscopic characterisation of the [D2,C,S] system: an update from the laboratory and theory

Natalia Inostroza-Pino, Valerio Lattanzi, C. Zachary Palmer +5

The synergy between high-resolution rotational spectroscopy and quantum-chemical calculations is essential for exploring future detection of molecules, especially when spectroscopy…

astro-ph.SR2019★ 74 cited

High sensitivity maps of molecular ions in L1544: I. Deuteration of N2H+ and HCO+ and first evidence of N2D+ depletion

Elena Redaelli, Luca Bizzocchi, Paola Caselli +4

Context. The deuterium fraction in low-mass prestellar cores is a good diagnostic indicator of the initial phases of star formations, and it is also a fundamental quantity to infer…

astro-ph.GA2018★ 55 cited

Mapping deuterated methanol toward L1544: I. Deuterium fraction and comparison with modeling

A. Chacon-Tanarro, P. Caselli, L. Bizzocchi +7

The study of deuteration in pre-stellar cores is important to understand the physical and chemical initial conditions in the process of star formation. In particular, observations…

astro-ph.GA2018★ 13 cited

Accurate millimetre and submillimetre rest frequencies for - and -dithioformic acid, HCSSH

D. Prudenzano, J. Laas, L. Bizzocchi +6

A better understanding of sulphur chemistry is needed to solve the interstellar sulphur depletion problem. A way to achieve this goal is to study new S-bearing molecules in the lab…

astro-ph.GA2017★ 87 cited

The observed chemical structure of L1544

S. Spezzano, P. Caselli, L. Bizzocchi +2

Prior to star formation, pre-stellar cores accumulate matter towards the centre. As a consequence, their central density increases while the temperature decreases. Understanding th…