Phenalene (C13H10) is detected for the first time outside TMC-1 CP, in the VeLLO MC27/L1521F, with a phenalene-to-benzonitrile ratio four times higher than in TMC-1 CP.
and Lee, Kin Long Kelvin and Changala, P
6 Pith papers cite this work, alongside 219 external citations. Polarity classification is still indexing.
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2026 6representative citing papers
Water binding energy on silicate grains is twice that on ice, enabling local retention and inheritance for terrestrial planets without outer Solar System delivery.
Experiments identify acenaphthene derivatives from C11H9+ reactivity with methylated naphthalenes and link them to efficient formation of acenaphthylene-like species in cold clouds.
Hydrogen tunneling makes H-abstraction reactions by C2H, OH, and CN competitive in TMC-1 despite low individual rates, affecting aromatic abundance predictions.
The CH₃OH/CH₃CN ratio in the S68N outflow is constant at ~100-200 and matches gas-phase astrochemical models only when cosmic-ray ionization rates are raised to ~10^{-14} s^{-1}.
SKA will detect emission from heavy molecules and prebiotic species in obscured disk regions to constrain initial chemical conditions for planet formation.
citing papers explorer
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Detection of the Polycyclic Aromatic Hydrocarbon Phenalene (C$_{13}$H$_{10}$) in the Very Low Luminosity Object (VeLLO) MC27/L1521F
Phenalene (C13H10) is detected for the first time outside TMC-1 CP, in the VeLLO MC27/L1521F, with a phenalene-to-benzonitrile ratio four times higher than in TMC-1 CP.
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Astrochemical Inheritance of Terrestrial Planets Water from Local Wet Silicates
Water binding energy on silicate grains is twice that on ice, enabling local retention and inheritance for terrestrial planets without outer Solar System delivery.
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Acenaphthene Derivatives as Signatures of C$_{11}$H$_9^+$ Reactivity with Methylated Naphthalenes
Experiments identify acenaphthene derivatives from C11H9+ reactivity with methylated naphthalenes and link them to efficient formation of acenaphthylene-like species in cold clouds.
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The impact of hydrogen atom tunneling on aromatic chemistry in TMC-1
Hydrogen tunneling makes H-abstraction reactions by C2H, OH, and CN competitive in TMC-1 despite low individual rates, affecting aromatic abundance predictions.
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Probing outflow physics through CH$_3$CN and CH$_3$OH chemistry
The CH₃OH/CH₃CN ratio in the S68N outflow is constant at ~100-200 and matches gas-phase astrochemical models only when cosmic-ray ionization rates are raised to ~10^{-14} s^{-1}.
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Unveiling Complex Chemistry in Planet-forming Disks with the SKAO
SKA will detect emission from heavy molecules and prebiotic species in obscured disk regions to constrain initial chemical conditions for planet formation.