Detection of C60 in embedded young stellar objects, a Herbig Ae/Be star and an unusual post-AGB star
arXiv:1201.3542 · doi:10.1111/j.1365-2966.2012.20552.x
Abstract
The first detection of the C60 (Buckminsterfullerene) molecule in massive embedded young stellar objects (YSOs) is reported. Observations with Spitzer IRS reveal the presence of C60 in YSOs ISOGAL-P J174639.6-284126 and SSTGC 372630 in the Central Molecular Zone in the Galactic centre, and in a YSO candidate, 2MASS J06314796+0419381, in the Rosette nebula. The first detection of C60 in a Herbig Ae/Be star, HD 97300, is also reported. These observations extend the range of astrophysical environments in which C60 is found to YSOs and a pre-main sequence star. C60 excitation and formation mechanisms are discussed in the context of these results, together with its presence and processes in post-AGB objects such as HR 4049.
Accepted for publication in MNRAS, modifications since v1: flux ratios, T values, fig.9. Comprises 10 pages and 9 figures
References in corpus (10)
- Formation of buckminsterfullerene (C60) in interstellar space
- Star Formation in the Central 400 pc of the Milky Way: Evidence for a Population of Massive YSOs
- Formation of fullerenes in H-containing Planetary Nebulae
- The formation of fullerenes: clues from new C60, C70, and (possible) planar C24 detections in Magellanic Cloud Planetary Nebulae
- Silicate features in Galactic and extragalactic post-AGB discs
- Point Sources from a Spitzer IRAC Survey of the Galactic Center
- The Evolution of Massive YSOs in the LMC: Part I. Identification and Spectral Classification
- Carbonaceous molecules in the oxygen-rich circumstellar environment of binary post-AGB stars: C_{60} fullerenes and polycyclic aromatic hydrocarbons
- Lack of PAH emission toward low-mass embedded young stellar objects
- A Spitzer Space Telescope survey of massive young stellar objects in the G333.2-0.4 giant molecular cloud
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- The formation of cosmic fullerenes from arophatic clusters
- Physical Properties of Fullerene-containing Galactic Planetary Nebulae
- Detection of Buckminsterfullerene emission in the diffuse interstellar medium
- Searching for stable fullerenes in space with computational chemistry
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- Threshold Energies for Single Carbon Knockout from Polycyclic Aromatic Hydrocarbons
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- C60 as a probe for astrophysical environments
- Search for Hydrogenated C (fulleranes) in Circumstellar Envelopes
- Nano carbon dust emission in proto-planetary disks: the aliphatic-aromatic components
- Detection of Cosmic Fullerenes in the Almahata Sitta Meteorite: Are They an Interstellar Heritage?
- Petroleum, coal and other organics in space
- Physical properties of the fullerene C60-containing planetary nebula SaSt 2-3
- The Gas-Rich Circumbinary Disk of HR 4049 I: A Detailed Study of the Mid-Infrared Spectrum
- Evolution of Fullerenes in Circumstellar Envelopes by Carbon Condensation: Insights from Reactive Molecular Dynamics Simulations
- Restructuring and destruction of hydrocarbon dust in the interstellar medium
- Fullerenes in the circumstellar medium of Herbig Ae/Be stars: Insights from the Spitzer mid-infrared spectral catalog
- Laboratory study of the formation of fullerene (from smaller to larger, C to C)/anthracene cluster cations in the gas phase
- On the formation of molecules and solid-state compounds from the AGB to the PN phases