The Missing Giant: Do FAST Spectroscopic Observations Reveal a Scarcity of Large Polycyclic Aromatic Hydrocarbons in Astronomical Environments?
Yi Shao, Yong Zhang, Xu-Jia Ouyang, Chuan-Peng Zhang

TL;DR
Using the FAST telescope, the study searched for large PAHs in space but found no evidence, suggesting they may not be the main carriers of unidentified infrared emission bands, challenging existing theories.
Contribution
First observational search for large quasi-symmetric PAHs with FAST, setting upper limits that challenge current theoretical abundance predictions.
Findings
No detection of large PAHs in the spectra.
Upper limits on PAH abundance are lower than theoretical predictions.
Results suggest large PAHs may not be primary UIE carriers.
Abstract
The search for large polycyclic aromatic hydrocarbons (PAHs) with over 100 carbon atoms is crucial to resolving the origin of unidentified infrared emission (UIE) bands. These bands are commonly observed in nebulae and the interstellar medium, yet their spectroscopic assignment has remained unknown for decades. Using the Five-hundred-meter Aperture Spherical Radio Telescope (FAST), the world's most sensitive instrument operating in the decimeter-wavelength range, we conducted a search for rotational transitions of large, quasi-symmetric PAHs. Our sample included two prototypical UIE sources, NGC 7027 and TMC-1, along with a non-UIE source, IRC+10216, for comparison. A matched filter technique was employed to isolate comb-like spectral features from quasi-symmetric PAHs containing 138 to 194 carbon atoms in the FAST spectra. This method significantly enhanced detection sensitivity to…
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Astro and Planetary Science · Astronomy and Astrophysical Research
