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dc.contributor.author |
Churyumov, K.I. |
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dc.contributor.author |
Lukyanyk, I.V. |
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dc.contributor.author |
Chubko, L.S. |
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dc.contributor.author |
Kleshchonok, V.V. |
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dc.contributor.author |
Berezhnoy, A.A. |
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dc.contributor.author |
Chavushyan, V.H. |
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dc.contributor.author |
Sandoval, L. |
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dc.contributor.author |
Palma, A. |
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dc.date.accessioned |
2015-04-03T19:47:33Z |
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dc.date.available |
2015-04-03T19:47:33Z |
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dc.date.issued |
2005 |
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dc.identifier.citation |
Exploration of spectra of periodic Comet 153P/Ikeya−Zhang / K.I. Churyumov, I.V. Lukyanyk, L.S. Chubko, V.V. Kleshchonok, A.A. Berezhnoy, V.H. Chavushyan, L. Sandoval, A. Palma // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 472-476. — Бібліогр.: 13 назв. — англ. |
uk_UA |
dc.identifier.issn |
0233-7665 |
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dc.identifier.uri |
http://dspace.nbuv.gov.ua/handle/123456789/79701 |
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dc.description.abstract |
We present preliminary results of study of middle-resolution optical spectra of Comet 153P/Ikeya–Zhang obtained on May 5, 2002 with the help of the 2.12-m reflector of the Guillermo Haro Astrophysical Observatory. Emission lines of the molecules C₂, C₃, CN, NH₂, CO (Asundi and triplet bands), and H₂O⁺ are identified in these spectra. On the basis of the intensity distribution along the slit of the spectrograph in C₂, C₃, CN emission lines we determined the velocities expansion and life times of these molecules. |
uk_UA |
dc.description.sponsorship |
Authors K. I. Churyumov, I. V. Lukyanyk, and V. V. Kleshchonok thank to the Fundamental Research State Fund of the Ministry of Ukraine for Education and Science (grant 2002) for support of our research in cometary physics area. |
uk_UA |
dc.language.iso |
en |
uk_UA |
dc.publisher |
Головна астрономічна обсерваторія НАН України |
uk_UA |
dc.relation.ispartof |
Кинематика и физика небесных тел |
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dc.subject |
MS5: Dynamics and Physics of Solar System Bodies |
uk_UA |
dc.title |
Exploration of spectra of periodic Comet 153P/Ikeya−Zhang |
uk_UA |
dc.type |
Article |
uk_UA |
dc.status |
published earlier |
uk_UA |
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