Search Publications

Deuterated Polycyclic Aromatic Hydrocarbons in the Interstellar Medium: The Aliphatic C-D Band Strengths
DOI: 10.3847/1538-4365/ace4c6 Bibcode: 2023ApJS..268...12Y

Li, Aigen; Yang, X. J.

Deuterium (D) was exclusively generated in the Big Bang, and the standard Big Bang nucleosynthesis (BBN) model predicts a primordial abundance of D/H ≈ 26 parts per million (ppm). As the Galaxy evolves, D/H gradually decreases because of astration. The Galactic chemical evolution (GCE) model predicts a present-day abundance of D/H ≳ 20 ppm. Howeve…

2023 The Astrophysical Journal Supplement Series
ISO AKARI 9
Aliphatics and Aromatics in the Universe: The Pre-JWST Era
DOI: 10.3847/1538-4365/acebe6 Bibcode: 2023ApJS..268...50Y

Li, Aigen; Yang, X. J.

The so-called "unidentified infrared emission" (UIE) features at 3.3, 6.2, 7.7, 8.6, and 11.3 µm ubiquitously seen in a wide variety of astrophysical regions are generally attributed to polycyclic aromatic hydrocarbon (PAH) molecules. Astronomical PAHs often have an aliphatic component (e.g., aliphatic sidegroups like methyl -CH3

2023 The Astrophysical Journal Supplement Series
ISO AKARI 8