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20152026
most citedA Theoretical Study on the Vibrational Spectra of PAH Molecules with Aliphatic Sidegroups

33 citations · 156 across the 13 of their papers we have counts for

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Showing astro-ph.SRShow all

7 papers · 1 filter

astro-ph.SR2023

Infrared spectral fingerprint of neutral and charged endo- and exohedral metallofullerenes

R. Barzaga, D. A. Garcia-Hernandez, S. Diaz-Tendero +5

Small metal-containing molecules have been detected and recognized as one of the hybrid species efficiently formed in space; especially in the circumstellar envelopes of evolved st…

astro-ph.SR2022★ 13 cited

On the presence of metallofullerenes in fullerene-rich circumstellar envelopes

R. Barzaga, D. A. Garcia-Hernandez, S. Diaz-Tendero +3

The presence of neutral C60 fullerenes in circumstellar environments has been firmly established by astronomical observations as well as laboratory experiments and quantum-chemistr…

astro-ph.SR2021★ 5 cited

Morphological study of the nested planetary nebula Hubble 12

Chih-Hao Hsia, Yong Zhang, SeyedAbdolreza Sadjadi +3

We present a visible-infrared imaging study of young planetary nebula (PN) Hubble 12 (Hb 12; PN G111.8-02.8) obtained with Hubble Space Telescope (HST) archival data and our own Ca…

astro-ph.SR2020★ 16 cited

Hydrogenated Fullerenes (Fulleranes) in Space

Yong Zhang, Seyedabdolreza Sadjadi, Chih-Hao Hsia

Since the first laboratory synthesis of C in 1985, fullerene-related species have been proposed to interpret various astronomical features. After more than 25 years' efforts…

astro-ph.SR2017★ 24 cited

Search for Hydrogenated C (fulleranes) in Circumstellar Envelopes

Yong Zhang, SeyedAbdolreza Sadjadi, Chih-Hao Hsia +1

The recent detection of fullerene (C) in space and the positive assignment of five diffuse interstellar bands to C reinforce the notion that fullerene-related compo…

astro-ph.SR2016★ 12 cited

The 6 m Feature as A Tracer of Aliphatic Components of Interstellar Carbonaceous Grains

Chih-Hao Hsia, Seyedabdolreza Sadjadi, Yong Zhang +1

An unidentified infrared emission (UIE) feature at 6.0 m is detected in a number of astronomical sources showing the UIE bands. In contrast to the previous suggestion that this…