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Pathway to the Identification of C60+ in Diffuse Interstellar Clouds
The origin of the attenuation of starlight in diffuse clouds in interstellar space at specific wavelengths ranging from the visible to the near-infrared has been unknown since the first astronomical observations around a century ago.
Katol Filipkowski
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The Diffuse Interstellar Bands
Annual Review of Astronomy and Astrophysics, 1995G H Herbig
exaly +2 more sources
The Helicenes: Potential Carriers of Diffuse Interstellar Bands
ACS Earth and Space Chemistry, 2021Jorge Ona Ruales +2 more
exaly
Infrared Diffuse Interstellar Bands in the Galactic Centre Region
Nature, 2011Diego de la Fuente +2 more
exaly
Constraining the Size of the Carrier of the λ5797.1 Diffuse Interstellar Band
Molecular Physics, 2015Jane Huang, Takeshi Oka
exaly
Spectrochimica Acta - Part A: Molecular and Biomolecular Spectroscopy, 2001
Theodore P. Snow, T P Snow
exaly
Theodore P. Snow, T P Snow
exaly
On the Discovery of the Diffuse Interstellar Bands
Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences, 2013Benjamin McCall, R Elizabeth Griffin
exaly
Possible Identification of the Diffuse Interstellar Absorption Band at 4430 Å
Nature, 1969W W Duley, W R M Graham
exaly
Diffuse Interstellar Bands — An Observational Review (Review)
Astronomische Nachrichten, 1989J Krełowski
exaly

