Peculiarities of gas and dust production rates in comets P/Halley (1986 III), P/Giacobini-Zinner (1985 XIII), P/Hartley-Good (1985 XVII) and P/Thiele (1985 XIX)
An IHW narrow‐band photometry of comets P/Halley (1986 III), P/Giacobini‐Zinner (1985 XIII), P/Hartley‐Good (1985 XVII) and P/Thiele (1985 XIX) is presented. Molecular column densities and production rates of CN, C2, and C3 species observed in the coma are calculated in the framework of the Haser mo...
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Veröffentlicht in: | Astronomische Nachrichten 1991, Vol.312 (6), p.385-391 |
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description | An IHW narrow‐band photometry of comets P/Halley (1986 III), P/Giacobini‐Zinner (1985 XIII), P/Hartley‐Good (1985 XVII) and P/Thiele (1985 XIX) is presented. Molecular column densities and production rates of CN, C2, and C3 species observed in the coma are calculated in the framework of the Haser model. A comparative analysis of gas and dust production rates in the atmospheres of these comets is given. The effective comet nuclear radii have been estimated by different methods: for comet P/Hartley‐Good Reff ∼ 1·7 km, for P/Thiele Reff ∼ 2 km and for P/Giacobini‐Zinner Reff ∼ 1·3 km. |
doi_str_mv | 10.1002/asna.2113120610 |
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I. ; Rosenbush, V. K.</creator><creatorcontrib>Churyumov, K. I. ; Rosenbush, V. K.</creatorcontrib><description>An IHW narrow‐band photometry of comets P/Halley (1986 III), P/Giacobini‐Zinner (1985 XIII), P/Hartley‐Good (1985 XVII) and P/Thiele (1985 XIX) is presented. Molecular column densities and production rates of CN, C2, and C3 species observed in the coma are calculated in the framework of the Haser model. A comparative analysis of gas and dust production rates in the atmospheres of these comets is given. The effective comet nuclear radii have been estimated by different methods: for comet P/Hartley‐Good Reff ∼ 1·7 km, for P/Thiele Reff ∼ 2 km and for P/Giacobini‐Zinner Reff ∼ 1·3 km.</description><identifier>ISSN: 0004-6337</identifier><identifier>EISSN: 1521-3994</identifier><identifier>DOI: 10.1002/asna.2113120610</identifier><identifier>CODEN: ASNAAN</identifier><language>eng</language><publisher>Altona: WILEY-VCH Verlag</publisher><subject>Astronomy ; Comets ; dust production rates ; Earth, ocean, space ; Exact sciences and technology ; gas production rates ; Interplanetary space ; Solar system</subject><ispartof>Astronomische Nachrichten, 1991, Vol.312 (6), p.385-391</ispartof><rights>Copyright © 1991 WILEY‐VCH Verlag GmbH & Co. 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I.</creatorcontrib><creatorcontrib>Rosenbush, V. K.</creatorcontrib><title>Peculiarities of gas and dust production rates in comets P/Halley (1986 III), P/Giacobini-Zinner (1985 XIII), P/Hartley-Good (1985 XVII) and P/Thiele (1985 XIX)</title><title>Astronomische Nachrichten</title><addtitle>Astron. Nachr</addtitle><description>An IHW narrow‐band photometry of comets P/Halley (1986 III), P/Giacobini‐Zinner (1985 XIII), P/Hartley‐Good (1985 XVII) and P/Thiele (1985 XIX) is presented. Molecular column densities and production rates of CN, C2, and C3 species observed in the coma are calculated in the framework of the Haser model. A comparative analysis of gas and dust production rates in the atmospheres of these comets is given. The effective comet nuclear radii have been estimated by different methods: for comet P/Hartley‐Good Reff ∼ 1·7 km, for P/Thiele Reff ∼ 2 km and for P/Giacobini‐Zinner Reff ∼ 1·3 km.</description><subject>Astronomy</subject><subject>Comets</subject><subject>dust production rates</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>gas production rates</subject><subject>Interplanetary space</subject><subject>Solar system</subject><issn>0004-6337</issn><issn>1521-3994</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1991</creationdate><recordtype>article</recordtype><recordid>eNqFkE1PGzEQhi3USqTQM1cfOIDEkvF6vesVp0DbJCqiqcJHxMXy11LDZjeyN2r5N_2pOISk4tTTaOZ9nxnNi9ABgVMCkPZlaORpSgglKeQEdlCPsJQktCyzD6gHAFmSU1rsok8hPMa2zFPSQ38nVi9rJ73rnA24rfCDDFg2Bptl6PDCt2apO9c22MsuGlyDdTu3XcCT_kjWtX3GR6TkOR6Px8cncTh0UrfKNS65d01j_avM8Gyjj6TvIpUM29ZstNuovd6c9K9_OVvbLTQ73kcfK1kH-_mt7qGbb1-vL0bJ5Y_h-GJwmWiaAyREASt5xYw1SplKGcYpTTNuc8YrzYDTjBcqukoqGVVADM81VaUprCkVZHQP9dd7tW9D8LYSC-_m0j8LAmIVsFgFLP4FHInDNbGQQcu68rLRLmwxRjgwVkTb2dr228W__7dVDKZXg3dHkjXtQmf_bGnpn0Re0IKJu6uhSCfnMP3-k4sv9AWywpZ-</recordid><startdate>1991</startdate><enddate>1991</enddate><creator>Churyumov, K. I.</creator><creator>Rosenbush, V. K.</creator><general>WILEY-VCH Verlag</general><general>WILEY‐VCH Verlag</general><general>Akademie Verlag</general><scope>BSCLL</scope><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>1991</creationdate><title>Peculiarities of gas and dust production rates in comets P/Halley (1986 III), P/Giacobini-Zinner (1985 XIII), P/Hartley-Good (1985 XVII) and P/Thiele (1985 XIX)</title><author>Churyumov, K. I. ; Rosenbush, V. K.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c3600-1b0598f5dedbbdfbd5833248e658fc5083487b1b093a53b01d86c3b9d7ed9b043</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1991</creationdate><topic>Astronomy</topic><topic>Comets</topic><topic>dust production rates</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>gas production rates</topic><topic>Interplanetary space</topic><topic>Solar system</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Churyumov, K. I.</creatorcontrib><creatorcontrib>Rosenbush, V. K.</creatorcontrib><collection>Istex</collection><collection>Pascal-Francis</collection><collection>CrossRef</collection><jtitle>Astronomische Nachrichten</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Churyumov, K. I.</au><au>Rosenbush, V. K.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Peculiarities of gas and dust production rates in comets P/Halley (1986 III), P/Giacobini-Zinner (1985 XIII), P/Hartley-Good (1985 XVII) and P/Thiele (1985 XIX)</atitle><jtitle>Astronomische Nachrichten</jtitle><addtitle>Astron. Nachr</addtitle><date>1991</date><risdate>1991</risdate><volume>312</volume><issue>6</issue><spage>385</spage><epage>391</epage><pages>385-391</pages><issn>0004-6337</issn><eissn>1521-3994</eissn><coden>ASNAAN</coden><abstract>An IHW narrow‐band photometry of comets P/Halley (1986 III), P/Giacobini‐Zinner (1985 XIII), P/Hartley‐Good (1985 XVII) and P/Thiele (1985 XIX) is presented. Molecular column densities and production rates of CN, C2, and C3 species observed in the coma are calculated in the framework of the Haser model. A comparative analysis of gas and dust production rates in the atmospheres of these comets is given. The effective comet nuclear radii have been estimated by different methods: for comet P/Hartley‐Good Reff ∼ 1·7 km, for P/Thiele Reff ∼ 2 km and for P/Giacobini‐Zinner Reff ∼ 1·3 km.</abstract><cop>Altona</cop><pub>WILEY-VCH Verlag</pub><doi>10.1002/asna.2113120610</doi><tpages>7</tpages></addata></record> |
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subjects | Astronomy Comets dust production rates Earth, ocean, space Exact sciences and technology gas production rates Interplanetary space Solar system |
title | Peculiarities of gas and dust production rates in comets P/Halley (1986 III), P/Giacobini-Zinner (1985 XIII), P/Hartley-Good (1985 XVII) and P/Thiele (1985 XIX) |
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