The wavelengths of the strongest absorptions in the electronic spectrum of C+60 have been determined by experimental investigation into the perturbation caused by the helium in the laboratory spectra of C+60 - Hen(n = 1–3). The extrapolation of these gives absorption bands of bare C+60 at 9348.4, 9365.2, 9427.8, 9577.0, and 9632.1 Å, with ±0.2 Å as the 2σ uncertainty. The laboratory data are compared with the complete set of astronomical observations reported in the literature. The spectral characteristics are found to be in agreement with five diffuse interstellar bands, for which the systematic uncertainties are larger than for the laboratory data
International audienceGas phase spectroscopic laboratory experiments for the buckminsterfullerene ca...
Galazutdinov et al. (2017) recently claimed that the relative strengths of the 9577 and 9632 Å diffu...
International audienceEmission of fullerenes in their infrared vibrational bands has been detected i...
Recent low-temperature laboratory measurements and astronomical observations have proved that the fu...
The diffuse interstellar bands are absorption lines seen towards reddened stars. None of the molecul...
Context. Insight into the conditions that drive the physics and chemistry in interstellar clouds is ...
Based on gas-phase laboratory spectra at 6 K, Campbell et al. confirmed that the diffuse interstella...
The origin of the attenuation of starlight in diffuse clouds in interstellar space at specific wavel...
Recent low-temperature laboratory measurements and astronomical observations have proved that the fu...
After the discovery of C$_{60}$,\footnote{H.~W.~Kroto, J.~R.~Heath, S.~C.~O'Brian, R.~E.~Curl \& R.~...
Based on gas-phase laboratory spectra at 6 K, Campbell et al. confirmed that the diffuse interstella...
High spectral resolution studies of the two Diffuse Interstellar Bands (DIB) previously assigned to ...
It has recently been suggested that the diffuse interstellar bands may be formed by ionized polyhedr...
Low-temp. gas-phase wavelengths and bandwidths for astronomical searches for C60 in the 2400-4100 Å ...
Laboratory measurements are reported that enable a more accurate determination of the characteristic...
International audienceGas phase spectroscopic laboratory experiments for the buckminsterfullerene ca...
Galazutdinov et al. (2017) recently claimed that the relative strengths of the 9577 and 9632 Å diffu...
International audienceEmission of fullerenes in their infrared vibrational bands has been detected i...
Recent low-temperature laboratory measurements and astronomical observations have proved that the fu...
The diffuse interstellar bands are absorption lines seen towards reddened stars. None of the molecul...
Context. Insight into the conditions that drive the physics and chemistry in interstellar clouds is ...
Based on gas-phase laboratory spectra at 6 K, Campbell et al. confirmed that the diffuse interstella...
The origin of the attenuation of starlight in diffuse clouds in interstellar space at specific wavel...
Recent low-temperature laboratory measurements and astronomical observations have proved that the fu...
After the discovery of C$_{60}$,\footnote{H.~W.~Kroto, J.~R.~Heath, S.~C.~O'Brian, R.~E.~Curl \& R.~...
Based on gas-phase laboratory spectra at 6 K, Campbell et al. confirmed that the diffuse interstella...
High spectral resolution studies of the two Diffuse Interstellar Bands (DIB) previously assigned to ...
It has recently been suggested that the diffuse interstellar bands may be formed by ionized polyhedr...
Low-temp. gas-phase wavelengths and bandwidths for astronomical searches for C60 in the 2400-4100 Å ...
Laboratory measurements are reported that enable a more accurate determination of the characteristic...
International audienceGas phase spectroscopic laboratory experiments for the buckminsterfullerene ca...
Galazutdinov et al. (2017) recently claimed that the relative strengths of the 9577 and 9632 Å diffu...
International audienceEmission of fullerenes in their infrared vibrational bands has been detected i...