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<oai_dc:dc xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:doc="http://www.lyncode.com/xoai" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:dc="http://purl.org/dc/elements/1.1/" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd"><identifier>I19-R120-10915-123645</identifier><datestamp>2021-08-27T20:08:47Z</datestamp>
<dc:identifier>http://sedici.unlp.edu.ar/handle/10915/123645</dc:identifier>
<dc:identifier>issn:0004-6361</dc:identifier>
<dc:identifier>issn:1432-0746</dc:identifier>
<dc:title>Dynamics of the Edgeworth-Kuiper Belt beyond 50 AU : Spread of a primordial thin disk</dc:title>
<dc:creator>Brunini, Adrián</dc:creator>
<dc:date>2002-11</dc:date>
<dc:date>2021-08-27T16:13:18Z</dc:date>
<dc:language>en</dc:language>
<dc:subject>Astronomía</dc:subject>
<dc:subject>Kuiper Belt</dc:subject>
<dc:subject>comets: general</dc:subject>
<dc:subject>solar system: general</dc:subject>
<dc:description>In this paper we report numerical simulations of the dynamical evolution of the region a &gt; 50 AU. We found that some dynamical effects such as high-order secular resonances with the rate of precession of Neptune's node of the form kΩ· − Ω·&lt;sub&gt;Nep&lt;/sub&gt; with k = 4,5, ... or combined mean motion resonances with Uranus and Neptune of the form kn&lt;sub&gt;N&lt;/sub&gt; + jn&lt;sub&gt;U&lt;/sub&gt; + mn ∼ 0 may increase the area of a very thin primordial disk in this region by a factor of up to 2 after 4.5 Gy of evolution.</dc:description>
<dc:description>Facultad de Ciencias Astronómicas y Geofísicas</dc:description>
<dc:description>Instituto de Astrofísica de La Plata</dc:description>
<dc:type>Articulo</dc:type>
<dc:type>Articulo</dc:type>
<dc:rights>http://creativecommons.org/licenses/by-nc-sa/4.0/</dc:rights>
<dc:rights>Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)</dc:rights>
<dc:format>application/pdf</dc:format>
<dc:format>1129-1134</dc:format>
</oai_dc:dc>

Datos convertidos

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        "I19-R120-10915-1236452021-08-27T20:08:47Z http:\/\/sedici.unlp.edu.ar\/handle\/10915\/123645 issn:0004-6361 issn:1432-0746 Dynamics of the Edgeworth-Kuiper Belt beyond 50 AU : Spread of a primordial thin disk Brunini, Adri\u00e1n 2002-11 2021-08-27T16:13:18Z en Astronom\u00eda Kuiper Belt comets: general solar system: general In this paper we report numerical simulations of the dynamical evolution of the region a > 50 AU. We found that some dynamical effects such as high-order secular resonances with the rate of precession of Neptune's node of the form k\u2126\u00b7 \u2212 \u2126\u00b7Nep<\/sub> with k = 4,5, ... or combined mean motion resonances with Uranus and Neptune of the form knN<\/sub> + jnU<\/sub> + mn \u223c 0 may increase the area of a very thin primordial disk in this region by a factor of up to 2 after 4.5 Gy of evolution. Facultad de Ciencias Astron\u00f3micas y Geof\u00edsicas Instituto de Astrof\u00edsica de La Plata Articulo Articulo http:\/\/creativecommons.org\/licenses\/by-nc-sa\/4.0\/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application\/pdf 1129-1134"
    ],
    "institution": [
        "Universidad Nacional de La Plata"
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    "repository_str": "R-120",
    "collection": [
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    "language": [
        "Ingl\u00e9s"
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    "topic": [
        "Astronom\u00eda",
        "Kuiper Belt",
        "comets: general",
        "solar system: general"
    ],
    "spellingShingle": [
        "Astronom\u00eda",
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        "Brunini, Adri\u00e1n",
        "Dynamics of the Edgeworth-Kuiper Belt beyond 50 AU : Spread of a primordial thin disk"
    ],
    "topic_facet": [
        "Astronom\u00eda",
        "Kuiper Belt",
        "comets: general",
        "solar system: general"
    ],
    "description": "In this paper we report numerical simulations of the dynamical evolution of the region a > 50 AU. We found that some dynamical effects such as high-order secular resonances with the rate of precession of Neptune's node of the form k\u2126\u00b7 \u2212 \u2126\u00b7Nep<\/sub> with k = 4,5, ... or combined mean motion resonances with Uranus and Neptune of the form knN<\/sub> + jnU<\/sub> + mn \u223c 0 may increase the area of a very thin primordial disk in this region by a factor of up to 2 after 4.5 Gy of evolution.",
    "format": [
        "Articulo",
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    "author": [
        "Brunini, Adri\u00e1n"
    ],
    "author_facet": [
        "Brunini, Adri\u00e1n"
    ],
    "author_sort": "Brunini, Adri\u00e1n",
    "title": "Dynamics of the Edgeworth-Kuiper Belt beyond 50 AU : Spread of a primordial thin disk",
    "title_short": "Dynamics of the Edgeworth-Kuiper Belt beyond 50 AU : Spread of a primordial thin disk",
    "title_full": "Dynamics of the Edgeworth-Kuiper Belt beyond 50 AU : Spread of a primordial thin disk",
    "title_fullStr": "Dynamics of the Edgeworth-Kuiper Belt beyond 50 AU : Spread of a primordial thin disk",
    "title_full_unstemmed": "Dynamics of the Edgeworth-Kuiper Belt beyond 50 AU : Spread of a primordial thin disk",
    "title_sort": "dynamics of the edgeworth-kuiper belt beyond 50 au : spread of a primordial thin disk",
    "publishDate": [
        "2002"
    ],
    "url": [
        "http:\/\/sedici.unlp.edu.ar\/handle\/10915\/123645"
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