We present here the 7.0-8.7 micron spectrum of the bright reflection nebula NGC 7023. Our observations are made with the Short Wavelength Spectrometer (SWS) on the European satellite Infrared Space Observatory (ISO). The vibrational bands of the ionized fullerene C60+ are expected at 7.11 and 7.51 microns, while those of the neutral fullerene C60 are expected at 7.0 and 8.45 microns. We estimate an upper limit in NGC 7023 for the C60+ abundance of <0.26% of the interstellar abundance of carbon, while C60 contains <0.27% of interstellar carbon
Based on gas-phase laboratory spectra at 6 K, Campbell et al. confirmed that the diffuse interstella...
We performed multiwavelength observations of the planetary nebula (PN) M1-11 and we obtained its ele...
Large organic molecules and carbon clusters are basic building blocks of life, but their existence i...
Author Institution: Astronomy Department, Ohio State University; Observatoire de Haute Provenece, F-...
The fullerene C_(60) has four infrared-active vibrational transitions at 7.0, 8.5, 17.4, and 18.9 μm...
The electronic spectrum of the fullerene dication C702+ has been measured in the gas phase at low te...
Buckminsterfullerene (C60) has recently been detected through its infrared emission bands in the int...
We present new data on the photodissociation regions associated with the reflection nebula NGC7023. ...
Context. Insight into the conditions that drive the physics and chemistry in interstellar clouds is ...
We present high-resolution (R ~ 15 000) VLT/UVES optical spectra of two planetary nebulae (PNe; Tc...
It has recently been suggested that the diffuse interstellar bands may be formed by ionized polyhedr...
© 2016 The Authors.The laboratory gas-phase spectrum recently published by Campbell et al. has reinv...
After the discovery of C$_{60}$,\footnote{H.~W.~Kroto, J.~R.~Heath, S.~C.~O'Brian, R.~E.~Curl \& R.~...
Recent low-temperature laboratory measurements and astronomical observations have proved that the fu...
We searched the Spitzer Space Telescope data archive for Galactic planetary nebulae (PNe), which sho...
Based on gas-phase laboratory spectra at 6 K, Campbell et al. confirmed that the diffuse interstella...
We performed multiwavelength observations of the planetary nebula (PN) M1-11 and we obtained its ele...
Large organic molecules and carbon clusters are basic building blocks of life, but their existence i...
Author Institution: Astronomy Department, Ohio State University; Observatoire de Haute Provenece, F-...
The fullerene C_(60) has four infrared-active vibrational transitions at 7.0, 8.5, 17.4, and 18.9 μm...
The electronic spectrum of the fullerene dication C702+ has been measured in the gas phase at low te...
Buckminsterfullerene (C60) has recently been detected through its infrared emission bands in the int...
We present new data on the photodissociation regions associated with the reflection nebula NGC7023. ...
Context. Insight into the conditions that drive the physics and chemistry in interstellar clouds is ...
We present high-resolution (R ~ 15 000) VLT/UVES optical spectra of two planetary nebulae (PNe; Tc...
It has recently been suggested that the diffuse interstellar bands may be formed by ionized polyhedr...
© 2016 The Authors.The laboratory gas-phase spectrum recently published by Campbell et al. has reinv...
After the discovery of C$_{60}$,\footnote{H.~W.~Kroto, J.~R.~Heath, S.~C.~O'Brian, R.~E.~Curl \& R.~...
Recent low-temperature laboratory measurements and astronomical observations have proved that the fu...
We searched the Spitzer Space Telescope data archive for Galactic planetary nebulae (PNe), which sho...
Based on gas-phase laboratory spectra at 6 K, Campbell et al. confirmed that the diffuse interstella...
We performed multiwavelength observations of the planetary nebula (PN) M1-11 and we obtained its ele...
Large organic molecules and carbon clusters are basic building blocks of life, but their existence i...