Astronomical School’s Report, 2004, Volume 5, Issue 1-2, Pages 111–114

https://doi.org/10.18372/2411-6602.05.1111
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UDC 52–16, 52–823, 520.84

Identification of emission lines in the spectrum of comet C/2002 V1 (NEAT)

Churiumov K.I.1, Luk’yanyk I.V.1, Kleschonok V.V.1, Chubko L.S.1, Berezhnoy A.A.2, Chavushyan V.Kh.3, Sandoval L.4, Pal’ma A.4

1Kyiv Shevchenko National University, Ukraine
2Sternberg Astronomical Institute, Russia
3National Institute of Astrophysics, Optics and Electronics, Tonantzintla, Mexico
4Meritorious Autonomous University of Puebla, Mexico

Abstract

Two of middle-resolution optical spectra of comet C/2002 V1 (NEAT) were obtained on 27 Jan. 2003 with the help of the 2.12-m reflector of the Guillermo Haro Astrophysical Observatory. Detailed identification of the spectral emission lines was made.

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References

  1. Brown M.E., Bouchez A.H., Spinrad H., Jons-Krull C.M., Astron. J, 1996, 112, No 3, P. 1197–1202. https://doi.org/10.1086/118090
  2. A.Cochran A high spectral resolution Atlas of comet 122P/de Vico. 2001. https://doi.org/10.1006/icar.2002.6850

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