First experimental determination of the [13C II] hyperfine-structure constants A1/2=810.71(11) MHz and A3/2=162.18(5) MHz from astronomical spectra.
Tracing the Formation of Molecular Clouds via [
2 Pith papers cite this work, alongside 99 external citations. Polarity classification is still indexing.
2
Pith papers citing it
99
external citations · OpenAlex
fields
astro-ph.GA 2years
2026 2representative citing papers
ALMA survey of CO(7-6) and [C I](2-1) in 18 z~6 quasars yields molecular gas mass estimates from multiple tracers and indicates that PDR models cannot fully account for the observed excitation, pointing to additional heating processes.
citing papers explorer
-
Space as a spectroscopic laboratory: High-resolution spectroscopy of the [$^{13}$C II] hyperfine structure with SOFIA/upGREAT
First experimental determination of the [13C II] hyperfine-structure constants A1/2=810.71(11) MHz and A3/2=162.18(5) MHz from astronomical spectra.
-
CO(7-6) and [C I](2-1) survey in z > 6 quasars
ALMA survey of CO(7-6) and [C I](2-1) in 18 z~6 quasars yields molecular gas mass estimates from multiple tracers and indicates that PDR models cannot fully account for the observed excitation, pointing to additional heating processes.