Unidentified Spectral Lines between 4800 and 8100 Å in High-Resolution Spectra of Comets

Details Unidentified Spectral Lines between 4800 and 8100 Å in High-Resolution Spectra of Comets Unidentified Spectral Lines between 4800 and 8100 Å in High-Resolution Spectra of Comets

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010dps....42.2816s&link_type=abstract

American Astronomical Society, DPS meeting #42, #28.16; Bulletin of the American Astronomical Society, Vol. 42, p.962

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Scientific paper

Visible spectrum of Comet Machholz (C/2004Q2) was obtained in the wavelength range of 2800 8100 Å with a resolution of 30,000 using BOES (BOao Echelle Spectograph) at Bohyunsan Observatory on January 4, 2005. It was found that emission lines of Machholz spectra were mostly originate from C2, NH2, CN, and H2O+. A list of unidentified spectral lines was compared with high-resolution visible spectra of other comets in literature: Swift-Tuttle, Brorsen-Metcalf, Austin, and 122P/de Vico. We will present identified molecular lines, which are previously unknown; and these identifications will be useful information for studying high-resolution spectra of future comets.

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