Stability constraints in modeling of multi-planet extrasolar systems
We present an analysis of high precision radial velocity (RV) observations of stars hosting multi-planet systems with Jovian companions. We use dynamical stability constraints and quasi-global methods of optimization. As an illustration, we present new results derived for the RV data of the Sun-like...
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creator | Gozdziewski, K Migaszewski, C Musielinski, A |
description | We present an analysis of high precision radial velocity (RV) observations of
stars hosting multi-planet systems with Jovian companions. We use dynamical
stability constraints and quasi-global methods of optimization. As an
illustration, we present new results derived for the RV data of the Sun-like
dwarfs HD 155358 and $\tau^1$ Gruis. |
doi_str_mv | 10.48550/arxiv.0802.0254 |
format | Article |
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stars hosting multi-planet systems with Jovian companions. We use dynamical
stability constraints and quasi-global methods of optimization. As an
illustration, we present new results derived for the RV data of the Sun-like
dwarfs HD 155358 and $\tau^1$ Gruis.</description><identifier>DOI: 10.48550/arxiv.0802.0254</identifier><language>eng</language><subject>Physics - Astrophysics of Galaxies ; Physics - Cosmology and Nongalactic Astrophysics ; Physics - Earth and Planetary Astrophysics ; Physics - High Energy Astrophysical Phenomena ; Physics - Instrumentation and Methods for Astrophysics ; Physics - Solar and Stellar Astrophysics</subject><creationdate>2008-02</creationdate><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,885</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/0802.0254$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.0802.0254$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Gozdziewski, K</creatorcontrib><creatorcontrib>Migaszewski, C</creatorcontrib><creatorcontrib>Musielinski, A</creatorcontrib><title>Stability constraints in modeling of multi-planet extrasolar systems</title><description>We present an analysis of high precision radial velocity (RV) observations of
stars hosting multi-planet systems with Jovian companions. We use dynamical
stability constraints and quasi-global methods of optimization. As an
illustration, we present new results derived for the RV data of the Sun-like
dwarfs HD 155358 and $\tau^1$ Gruis.</description><subject>Physics - Astrophysics of Galaxies</subject><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><subject>Physics - Earth and Planetary Astrophysics</subject><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><subject>Physics - Solar and Stellar Astrophysics</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2008</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotzz1PwzAUhWEvDKhlZ0L-AwlO7JvcjFX5lCox0D26dmxkyXEq26Dm30OB6SyvjvQwdtuIWiGAuKd09l-1QNHWogV1zR7eC2kffFm5WWIuiXwsmfvI52WywccPvjg-f4biq1OgaAu3558qL4ESz2suds5bduUoZHvzvxt2fHo87l-qw9vz6353qKgDVZFpEFFj64xxwwTkAKhvCaF3qK1RBslhb6xoOhKSOiOHSSvZ6cb0MDi5YXd_t7-K8ZT8TGkdL5rxopHf4D5G1w</recordid><startdate>20080202</startdate><enddate>20080202</enddate><creator>Gozdziewski, K</creator><creator>Migaszewski, C</creator><creator>Musielinski, A</creator><scope>GOX</scope></search><sort><creationdate>20080202</creationdate><title>Stability constraints in modeling of multi-planet extrasolar systems</title><author>Gozdziewski, K ; Migaszewski, C ; Musielinski, A</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a654-ac1888b82fccf9d5af55a72a857f8bec4c8af87ce016a03a6c39db436b1c759f3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2008</creationdate><topic>Physics - Astrophysics of Galaxies</topic><topic>Physics - Cosmology and Nongalactic Astrophysics</topic><topic>Physics - Earth and Planetary Astrophysics</topic><topic>Physics - High Energy Astrophysical Phenomena</topic><topic>Physics - Instrumentation and Methods for Astrophysics</topic><topic>Physics - Solar and Stellar Astrophysics</topic><toplevel>online_resources</toplevel><creatorcontrib>Gozdziewski, K</creatorcontrib><creatorcontrib>Migaszewski, C</creatorcontrib><creatorcontrib>Musielinski, A</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Gozdziewski, K</au><au>Migaszewski, C</au><au>Musielinski, A</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Stability constraints in modeling of multi-planet extrasolar systems</atitle><date>2008-02-02</date><risdate>2008</risdate><abstract>We present an analysis of high precision radial velocity (RV) observations of
stars hosting multi-planet systems with Jovian companions. We use dynamical
stability constraints and quasi-global methods of optimization. As an
illustration, we present new results derived for the RV data of the Sun-like
dwarfs HD 155358 and $\tau^1$ Gruis.</abstract><doi>10.48550/arxiv.0802.0254</doi><oa>free_for_read</oa></addata></record> |
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subjects | Physics - Astrophysics of Galaxies Physics - Cosmology and Nongalactic Astrophysics Physics - Earth and Planetary Astrophysics Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics Physics - Solar and Stellar Astrophysics |
title | Stability constraints in modeling of multi-planet extrasolar systems |
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