On changes in the spectra of Comet C/1999 S4 (LINEAR) on July 22−28, 2002

Some spectra of Comet C/1999 S4 (LINEAR) are obtained with the UAGS spectrograph (long slit and CCD) installed on the 1-m Zeiss reflector of the SAO RAS (the Northern Caucasus, Nizhny Arkhyz) on July 23/24, 26/27, and 27/28, 2000. Sophisticated identification of emission lines in the spectra of Come...

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Veröffentlicht in:Кинематика и физика небесных тел
Datum:2005
Hauptverfasser: Chubko, L.S., Churyumov, K.I., Lukyanyk, I.V., Kleshchonok, V.V.
Format: Artikel
Sprache:Englisch
Veröffentlicht: Головна астрономічна обсерваторія НАН України 2005
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Online Zugang:https://nasplib.isofts.kiev.ua/handle/123456789/79710
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Zitieren:On changes in the spectra of Comet C/1999 S4 (LINEAR) on July 22−28, 2002 / L.S. Chubko, K.I. Churyumov, I.V. Lukyanyk, V.V. Kleshchonok // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 504-508. — Бібліогр.: 8 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
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author Chubko, L.S.
Churyumov, K.I.
Lukyanyk, I.V.
Kleshchonok, V.V.
author_facet Chubko, L.S.
Churyumov, K.I.
Lukyanyk, I.V.
Kleshchonok, V.V.
citation_txt On changes in the spectra of Comet C/1999 S4 (LINEAR) on July 22−28, 2002 / L.S. Chubko, K.I. Churyumov, I.V. Lukyanyk, V.V. Kleshchonok // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 504-508. — Бібліогр.: 8 назв. — англ.
collection DSpace DC
container_title Кинематика и физика небесных тел
description Some spectra of Comet C/1999 S4 (LINEAR) are obtained with the UAGS spectrograph (long slit and CCD) installed on the 1-m Zeiss reflector of the SAO RAS (the Northern Caucasus, Nizhny Arkhyz) on July 23/24, 26/27, and 27/28, 2000. Sophisticated identification of emission lines in the spectra of Comet C/1999 S4 (LINEAR) is made. Emission lines of the molecules C₂, C₃, CN, NH, CH, NH₂, CO⁺, H₂O⁺, and others were identified in the spectra of Comet C/1999 S4 (LINEAR) derived on July 22/23, 2000 before splitting the cometary nucleus. Analysis of the CCD spectra obtained on July 27/28, 2000 reveals very weak emission lines superposed on the solar reflection spectrum, unlike the case of spectra obtained with the same instrument on July 22/23. From analysis of the surface brightness profile of C₂ along the slit, the velocity of expansion of two secondary fragments (V = 10 km/hr) and energy of fragment expansion (E = 8.7 · 10¹⁵ erg) are estimated. The luminescence cometary continuum is detected by a level of 26% at 5000 Å in the spectra of the comet. Possible mechanisms of nucleus splitting are discussed.
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spelling Chubko, L.S.
Churyumov, K.I.
Lukyanyk, I.V.
Kleshchonok, V.V.
2015-04-03T20:00:34Z
2015-04-03T20:00:34Z
2005
On changes in the spectra of Comet C/1999 S4 (LINEAR) on July 22−28, 2002 / L.S. Chubko, K.I. Churyumov, I.V. Lukyanyk, V.V. Kleshchonok // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 504-508. — Бібліогр.: 8 назв. — англ.
0233-7665
https://nasplib.isofts.kiev.ua/handle/123456789/79710
Some spectra of Comet C/1999 S4 (LINEAR) are obtained with the UAGS spectrograph (long slit and CCD) installed on the 1-m Zeiss reflector of the SAO RAS (the Northern Caucasus, Nizhny Arkhyz) on July 23/24, 26/27, and 27/28, 2000. Sophisticated identification of emission lines in the spectra of Comet C/1999 S4 (LINEAR) is made. Emission lines of the molecules C₂, C₃, CN, NH, CH, NH₂, CO⁺, H₂O⁺, and others were identified in the spectra of Comet C/1999 S4 (LINEAR) derived on July 22/23, 2000 before splitting the cometary nucleus. Analysis of the CCD spectra obtained on July 27/28, 2000 reveals very weak emission lines superposed on the solar reflection spectrum, unlike the case of spectra obtained with the same instrument on July 22/23. From analysis of the surface brightness profile of C₂ along the slit, the velocity of expansion of two secondary fragments (V = 10 km/hr) and energy of fragment expansion (E = 8.7 · 10¹⁵ erg) are estimated. The luminescence cometary continuum is detected by a level of 26% at 5000 Å in the spectra of the comet. Possible mechanisms of nucleus splitting are discussed.
en
Головна астрономічна обсерваторія НАН України
Кинематика и физика небесных тел
MS5: Dynamics and Physics of Solar System Bodies
On changes in the spectra of Comet C/1999 S4 (LINEAR) on July 22−28, 2002
Article
published earlier
spellingShingle On changes in the spectra of Comet C/1999 S4 (LINEAR) on July 22−28, 2002
Chubko, L.S.
Churyumov, K.I.
Lukyanyk, I.V.
Kleshchonok, V.V.
MS5: Dynamics and Physics of Solar System Bodies
title On changes in the spectra of Comet C/1999 S4 (LINEAR) on July 22−28, 2002
title_full On changes in the spectra of Comet C/1999 S4 (LINEAR) on July 22−28, 2002
title_fullStr On changes in the spectra of Comet C/1999 S4 (LINEAR) on July 22−28, 2002
title_full_unstemmed On changes in the spectra of Comet C/1999 S4 (LINEAR) on July 22−28, 2002
title_short On changes in the spectra of Comet C/1999 S4 (LINEAR) on July 22−28, 2002
title_sort on changes in the spectra of comet c/1999 s4 (linear) on july 22−28, 2002
topic MS5: Dynamics and Physics of Solar System Bodies
topic_facet MS5: Dynamics and Physics of Solar System Bodies
url https://nasplib.isofts.kiev.ua/handle/123456789/79710
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