Interstellar C_2 Molecule Detected in UV Spectra of Reddened Stars

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dc.creatorDyrka, M.
dc.creatorWszolek, B.
dc.date2007-12-10
dc.date.accessioned2026-07-07T08:48:15Z
dc.date.available2026-07-07T08:48:15Z
dc.description$C_2$ molecule is sometimes considered as a crucial component of carriers of some diffuse interstellar bands. Using UV data achieved by spectrometer STIS fed with HST we detected interstellar $C_2$ lines for few reddened target stars. We tried to verify the idea that intensity of $C_2$ lines around 2313 Åis correlated with some diffuse interstellar bands.
dc.descriptionPublished in Proceedings of the 14th Young Scientists Conference on Astronomy and Space Physics, Kyiv, Ukraine, April 23-28, 2007
dc.identifierhttps://arxiv.org/abs/0712.1452
dc.identifierhttp://arxiv.org/abs/0712.1452
dc.identifierYSC'14 Proceedings of Contributed Papers (eds. G. Ivashchenko, A. Golovin), Kyiv, Kyivskyi Universytet, pp. 30-33, 2007
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/143883
dc.subjectAstrophysics
dc.titleInterstellar C_2 Molecule Detected in UV Spectra of Reddened Stars
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