Changes in the spectra of comet C/1999 S4 in July, 2000

Details Changes in the spectra of comet C/1999 S4 in July, 2000 Changes in the spectra of comet C/1999 S4 in July, 2000

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005hia....13r.768c&link_type=abstract

In: Highlights of Astronomy, Vol. 13, as presented at the XXVth General Assembly of the IAU - 2003 [Sydney, Australia, 13 - 26 J

Astronomy and Astrophysics

Astronomy

Comets, Spectra

Scientific paper

The spectra of comet C/1999 S4 (LINEAR) were obtained with the eshelle-spectrograph (and CCD) installed on the 2-m Zeiss reflector of the Shamakhy Astronomical Observatory of the Azerbajan Academy of Sciences (Mount Pirkuli) on July 21 and 23 2000. The spectra of comet C/1999 S4 (LINEAR) were also obtained with the UAGS spectrograph (long slit and CCD) installed on the 1-m Zeiss reflector of the SAO of the RAS (Northern Caucasus Nizhny Arkhyz) on July 23 27 and 28 2000. Emissions lines of the molecules C2 C3 CN NH CH NH2 CO CO+ H2O+and other were identified in the spectra of comet C/1999 S4 obtained on July 21 23 and 27 2000 during splitting of the cometary nucleus. Changes in the spectra are discussed.

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