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20112026
most citedSurviving the hole I: Spatially resolved chemistry around Sgr A*

76 citations · 156 across the 8 of their papers we have counts for

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Showing 2026Show all

6 papers · 1 filter

astro-ph.IM2026

Chemical Demographics of Star-forming Regions

Maria N. Drozdovskaya, Timea Csengeri, Maria Teresa Beltrán +35

Our understanding of complex organic chemistry during the formation of stars and planets is shaped by a handful of cherry-picked sources with bright molecular emission lines. This…

astro-ph.IM2026

Star Formation across the Galaxy

Alvaro Sanchez-Monge, Henrik Beuther, Maryvonne Gerin +41

Star formation is both a multi-scale and highly dynamic process. It is regulated by the combination of gravity, turbulence, feedback and magnetic fields, which connect more than si…

astro-ph.IM2026

Frontiers of chemical complexity in the interstellar medium: unveiling the cosmic origins of life

Víctor M. Rivilla, Miguel Sanz-Novo, Maite Beltrán +33

The interstellar medium (ISM) contains a rich molecular inventory that provides a unique window into the chemistry operating during star and planet formation and its connection to…

astro-ph.IM2026

From local chemistry to galactic evolution: unlocking the power of interstellar isotopes with ALMA2040

Laura Colzi, Hayley A. Bunn, Víctor M. Rivilla +29

Molecular isotopic ratios provide a unique window into the chemical evolution of the interstellar medium, linking stellar nucleosynthesis and Galactic chemical evolution to the phy…

astro-ph.IM2026

Molecular atlas of nearby galaxies through sensitive high-resolution multi-band molecular line surveys

Mathilde Bouvier, Erica Behrens, Laura Colzi +21

Star formation and associated feedback processes play a key role in galaxy evolution. Astrochemistry is a powerful tool for characterising the physical conditions of dense star-for…

astro-ph.GA2026

ACES VII. Compact Continuum Source Catalog of the Central Molecular Zone

Jennifer Wallace, Cara Battersby, Nazar Budaiev +58

The Central Molecular Zone (CMZ) resides in the inner few hundred parsecs of our Galaxy, and despite being the largest reservoir of dense molecular gas in the Milky Way, it has a r…