Gas and dust in Comet 2P/Encke observed in the visual and submillimeter wavelength ranges
In November 2003 Comet 2P/Encke was observed simultaneously with the 10-m Heinrich–Hertz Submillimeter Telescope on Mount Graham, Arizona, USA, and the 2-m optical telescope on Mount Rozhen, Bulgaria. Simultaneous radio observations of the 4–3 and 3–2 rotational transitions of HCN and the 0–0 transi...
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Дата: | 2005 |
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Головна астрономічна обсерваторія НАН України
2005
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Назва видання: | Кинематика и физика небесных тел |
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Онлайн доступ: | http://dspace.nbuv.gov.ua/handle/123456789/79699 |
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Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
Цитувати: | Gas and dust in Comet 2P/Encke observed in the visual and submillimeter wavelength ranges / K. Jockers, S. Szutowicz, G. Villanueva, N. Kiselev, T. Bonev, P. Hartogh // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 458-464. — Бібліогр.: 18 назв. — англ. |
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irk-123456789-796992015-04-04T03:02:33Z Gas and dust in Comet 2P/Encke observed in the visual and submillimeter wavelength ranges Jockers, K. Szutowicz, S. Villanueva, G. Kiselev, N. Bonev, T. Hartogh, P. MS5: Dynamics and Physics of Solar System Bodies In November 2003 Comet 2P/Encke was observed simultaneously with the 10-m Heinrich–Hertz Submillimeter Telescope on Mount Graham, Arizona, USA, and the 2-m optical telescope on Mount Rozhen, Bulgaria. Simultaneous radio observations of the 4–3 and 3–2 rotational transitions of HCN and the 0–0 transition of the CN violet band system provide a three-dimensional view on the comet. The observations are consistent with outgassing from the source region I with location and pole position of Comet Encke taken from [14]. The outflow speed is 1.2 km. There is some evidence for another possible parent for CN besides HCN. The visual dust coma of Comet Encke is nearly spherical with a diameter of about 1000 km and a slight extension into Comet Encke’s fan. The polarization of the observed NH₂ transition at 662 nm is 7% at a phase angle of 94.5°, close to the value for two-atomic molecules. At this phase angle and a wavelength of 642 nm the polarization of Comet Encke’s dust is greater than 30%, i.e., exceeds the value for so-called dusty comets. 2005 Article Gas and dust in Comet 2P/Encke observed in the visual and submillimeter wavelength ranges / K. Jockers, S. Szutowicz, G. Villanueva, N. Kiselev, T. Bonev, P. Hartogh // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 458-464. — Бібліогр.: 18 назв. — англ. 0233-7665 http://dspace.nbuv.gov.ua/handle/123456789/79699 en Кинематика и физика небесных тел Головна астрономічна обсерваторія НАН України |
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Digital Library of Periodicals of National Academy of Sciences of Ukraine |
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English |
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MS5: Dynamics and Physics of Solar System Bodies MS5: Dynamics and Physics of Solar System Bodies |
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MS5: Dynamics and Physics of Solar System Bodies MS5: Dynamics and Physics of Solar System Bodies Jockers, K. Szutowicz, S. Villanueva, G. Kiselev, N. Bonev, T. Hartogh, P. Gas and dust in Comet 2P/Encke observed in the visual and submillimeter wavelength ranges Кинематика и физика небесных тел |
description |
In November 2003 Comet 2P/Encke was observed simultaneously with the 10-m Heinrich–Hertz Submillimeter Telescope on Mount Graham, Arizona, USA, and the 2-m optical telescope on Mount Rozhen, Bulgaria. Simultaneous radio observations of the 4–3 and 3–2 rotational transitions of HCN and the 0–0 transition of the CN violet band system provide a three-dimensional view on the comet. The observations are consistent with outgassing from the source region I with location and pole position of Comet Encke taken from [14]. The outflow speed is 1.2 km. There is some evidence for another possible parent for CN besides HCN. The visual dust coma of Comet Encke is nearly spherical with a diameter of about 1000 km and a slight extension into Comet Encke’s fan. The polarization of the observed NH₂ transition at 662 nm is 7% at a phase angle of 94.5°, close to the value for two-atomic molecules. At this phase angle and a wavelength of 642 nm the polarization of Comet Encke’s dust is greater than 30%, i.e., exceeds the value for so-called dusty comets. |
format |
Article |
author |
Jockers, K. Szutowicz, S. Villanueva, G. Kiselev, N. Bonev, T. Hartogh, P. |
author_facet |
Jockers, K. Szutowicz, S. Villanueva, G. Kiselev, N. Bonev, T. Hartogh, P. |
author_sort |
Jockers, K. |
title |
Gas and dust in Comet 2P/Encke observed in the visual and submillimeter wavelength ranges |
title_short |
Gas and dust in Comet 2P/Encke observed in the visual and submillimeter wavelength ranges |
title_full |
Gas and dust in Comet 2P/Encke observed in the visual and submillimeter wavelength ranges |
title_fullStr |
Gas and dust in Comet 2P/Encke observed in the visual and submillimeter wavelength ranges |
title_full_unstemmed |
Gas and dust in Comet 2P/Encke observed in the visual and submillimeter wavelength ranges |
title_sort |
gas and dust in comet 2p/encke observed in the visual and submillimeter wavelength ranges |
publisher |
Головна астрономічна обсерваторія НАН України |
publishDate |
2005 |
topic_facet |
MS5: Dynamics and Physics of Solar System Bodies |
url |
http://dspace.nbuv.gov.ua/handle/123456789/79699 |
citation_txt |
Gas and dust in Comet 2P/Encke observed in the visual and submillimeter wavelength ranges / K. Jockers, S. Szutowicz, G. Villanueva, N. Kiselev, T. Bonev, P. Hartogh // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 458-464. — Бібліогр.: 18 назв. — англ. |
series |
Кинематика и физика небесных тел |
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first_indexed |
2023-10-18T19:19:18Z |
last_indexed |
2023-10-18T19:19:18Z |
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