activity
20162026
most citedFilamentary Accretion Flows in the Infrared Dark Cloud G14.225-0.506 Revealed by ALMA

102 citations · 412 across the 27 of their papers we have counts for

collaborators
Showing 2025Show all

8 papers · 1 filter

astro-ph.GA2025

First mapping of prebiotic molecule CH2NH in a pre-stellar core

Yuxin Lin, Silvia Spezzano, Olli Sipilä +2

We present the first spatially resolved map of methanimine CH2NH in the prestellar core L1544 using the IRAM 30m telescope. The 2-1 line at 127 GHz was mapped with…

astro-ph.GA2025★ 1 cited

High deuteration of methanol in L1544

S. Spezzano, W. Riedel, P. Caselli +7

Isotopic fractionation is a very powerful tool to follow the evolution of material from one stage to the next in the star-formation process. Pre-stellar cores exhibit some of the h…

astro-ph.GA2025

Tails of Gravity: Persistence of Star Formation in the CMZ Environment

Linjing Feng, Sihan Jiao, Fengwei Xu +16

We characterize star-forming gas in six molecular clouds (Sgr B1-off, Sgr B2, Sgr C, the 20 km s and 50 km s molecular clouds, and the Brick) in the Galactic central…

astro-ph.GA2025

Deep Andromeda JCMT-SCUBA2 Observations. The Submillimeter Maps and Giant Molecular Clouds

Sihan Jiao, Jingwen Wu, Hauyu Baobab Liu +23

We have carried out unprecedentedly deep, nearly confusion-limited JCMT-SCUBA2 mapping observations on the nearest spiral galaxy, M31 (Andromeda). The 850 m image with a 5…

astro-ph.GA2025★ 6 cited

Nascent chemical complexity in prestellar core IRAS 16293E: complex organics and deuterated methanol

Samantha Scibelli, Maria N. Drozdovskaya, Paola Caselli +5

Prestellar cores represent early sites of low-mass ( few M) star and planet formation and provide insight into initial chemical conditions of complex organic mole…

astro-ph.GA2025

Why is the Star Formation Rate Proportional to Dense Gas Mass?

Sihan Jiao, Fengwei Xu, Hauyu Baobab Liu +14

One of the most profound empirical laws of star formation is the Gao-Solomon relation, a linear correlation between the star formation rate (SFR) and the dense molecular gas mass.…

astro-ph.GA2025★ 8 cited

Gravitationally Bound Gas Determines Star Formation in the Galaxy

Sihan Jiao, Jingwen Wu, Zhi-Yu Zhang +13

Stars form from molecular gas under complex conditions influenced by multiple competing physical mechanisms, such as gravity, turbulence, and magnetic fields. However, accurately i…

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…