Detection of C60 and C70 in a Young Planetary Nebula

By J. Cami, Jeronimo Bernard-Salas, E. Peeters, S. E. Malek. Science, 2010

676 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Organic Chemistry

View Paper: https://www.semanticscholar.org/paper/c14ba4455e17f5045539de4a2d78bcf19825ce38

How researchers see this paper

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In Astronomy and Astrophysics

1. R. Garrod
2. E. Herbst
3. S. Ioppolo
4. H. Cuppen
5. C. Walsh
6. B. McGuire
7. D. Semenov
8. T. Lamberts

In Organic Chemistry

1. B. McGuire
2. R. Garrod
3. E. Herbst
4. H. Cuppen
5. A. Tielens

Citations in the corpus

• FORMATION OF FULLERENES IN H-CONTAINING PLANETARY NEBULAE (2010, methodology): “The infrared detection of C60 and C70 fullerenes in the PN Tc 1 (Cami et al. 2010) has been reported recently.”
• Mass loss of stars on the asymptotic giant branch (2018, background): “1993), and even fullerenes (C60 and C70) have been detected (Cami et al. 2010; Sloan et al. 2014). The CSE dust constitutes about one percent or less of the total circumstellar mass. Yet, the dust provides large diagnostic capacity, and it plays a major dynamic role. As for the gas, the dust composi”
• Discovery of the Pure Polycyclic Aromatic Hydrocarbon Indene (c-C9H8) with GOTHAM Observations of TMC-1 (2021, background): “…single infrared vibrational transition of the simplest aromatic molecule, benzene (c-C6H6), has been detected toward a handful of evolved sources (Cernicharo et al. 2001; Cami et al. 2010; Berné et al. 2013), but has limited utility as atmospheric absorption prevents its ground-based observability.”
• 2018 Census of Interstellar, Circumstellar, Extragalactic, Protoplanetary Disk, and Exoplanetary Molecules (2018, background): “C70 (rugbyballene) Cami et al. (2010) reported the detection of C70 in Spitzer observations of Tc 1.”
• Grain Surface Models and Data for Astrochemistry (2017, background): “These include highly-unsaturated carbon chains and cages, e.g., HC11N (Bell et al. 1997), and the fullerenes, C60, C60 +, and C70 (Cami et al. 2010; Berné et al. 2013; Campbell et al. 2015), the latter of which are also the largest molecular species discovered to date in the ISM.”