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Updated: Nov 12, 2025

Chromatographic Fingerprinting by Template Matching for Data Collected by Comprehensive Two-Dimensional Gas Chromatography
Published on: September 2, 2020
Detection of two interstellar polycyclic aromatic hydrocarbons via spectral matched filtering
Brett A McGuire1,2,3, Ryan A Loomis2, Andrew M Burkhardt3
1Department of Chemistry, Massachusetts Institute of Technology, Cambridge, MA 02139, USA. brettmc@mit.edu.
Astronomers detected specific polycyclic aromatic hydrocarbon (PAH) molecules, 1- and 2-cyanonaphthalene, in interstellar space using radio telescope data. This marks the first identification of individual PAH species responsible for ubiquitous infrared emission bands.
Area of Science:
- Astrochemistry
- Interstellar Medium Composition
- Astrobiology
Background:
- Unidentified infrared emission bands are common in astronomical sources.
- These bands are often attributed to polycyclic aromatic hydrocarbons (PAHs).
- No specific PAH molecule had been definitively identified in space until now.
Purpose of the Study:
- To identify specific polycyclic aromatic hydrocarbon (PAH) molecules in the interstellar medium.
- To investigate the origins of unidentified infrared emission bands.
- To explore in situ gas-phase PAH formation pathways.
Main Methods:
- Spectral matched filtering of radio data.
- Utilized the Green Bank Telescope for observations.
- Analysis focused on the TMC-1 molecular cloud.
Main Results:
- Detection of two nitrile-group-functionalized PAHs: 1-cyanonaphthalene and 2-cyanonaphthalene.
- Both identified molecules are bicyclic ring structures.
- These are the first specific PAH species identified in the interstellar medium.
Conclusions:
- The identified molecules contribute to the understanding of interstellar chemistry.
- Provides observational evidence for specific PAHs in space.
- Opens avenues for studying PAH formation and evolution.
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