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

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.

Bibliographic Details
Main Authors: K. I. Churiumov, I. V. Luk’yanyk, V. V. Kleschonok, L. S. Chubko, A. A. Berezhnoy, V. Kh. Chavushyan, L. Sandoval, A. Pal’ma
Format: Article
Language:English
Published: National Aviation University 2004-12-01
Series:Вісник Астрономічної школи
Online Access:http://astro.nau.edu.ua/issues/2004_V.5_Iss.1-2/111.html

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