FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3017797997> ?p ?o ?g. }

• W3017797997 endingPage "4655" @default.
• W3017797997 startingPage "4645" @default.
• W3017797997 abstract "ABSTRACT We study the orbital stability of a non-zero mass, close-in circular orbit planet around an eccentric orbit binary for various initial values of the binary eccentricity, binary mass fraction, planet mass, planet semimajor axis, and planet inclination by means of numerical simulations that cover 5 × 104 binary orbits. For small binary eccentricity, the stable orbits that extend closest to the binary (most stable orbits) are nearly retrograde and circulating. For high binary eccentricity, the most stable orbits are highly inclined and librate near the so-called generalized polar orbit which is a stationary orbit that is fixed in the frame of the binary orbit. For more extreme mass ratio binaries, there is a greater variation in the size of the stability region (defined by initial orbital radius and inclination) with planet mass and initial inclination, especially for low binary eccentricity. For low binary eccentricity, inclined planet orbits may be unstable even at large orbital radii (separation ${gt}5 , a_{rm b}$). The escape time for an unstable planet is generally shorter around an equal mass binary compared with an unequal mass binary. Our results have implications for circumbinary planet formation and evolution and will be helpful for understanding future circumbinary planet observations." @default.
• W3017797997 created "2020-05-01" @default.
• W3017797997 creator A5014975239 @default.
• W3017797997 creator A5051918386 @default.
• W3017797997 creator A5057592704 @default.
• W3017797997 date "2020-04-20" @default.
• W3017797997 modified "2023-10-11" @default.
• W3017797997 title "Polar planets around highly eccentric binaries are the most stable" @default.
• W3017797997 cites W1668843955 @default.
• W3017797997 cites W1770103633 @default.
• W3017797997 cites W1835005408 @default.
• W3017797997 cites W1856590628 @default.
• W3017797997 cites W1864108573 @default.
• W3017797997 cites W1887045015 @default.
• W3017797997 cites W1939384555 @default.
• W3017797997 cites W1969397443 @default.
• W3017797997 cites W1990703493 @default.
• W3017797997 cites W1996022818 @default.
• W3017797997 cites W2014498975 @default.
• W3017797997 cites W2031837501 @default.
• W3017797997 cites W2038524664 @default.
• W3017797997 cites W2045585206 @default.
• W3017797997 cites W2056285875 @default.
• W3017797997 cites W2065809336 @default.
• W3017797997 cites W2070154021 @default.
• W3017797997 cites W2080131766 @default.
• W3017797997 cites W2104198143 @default.
• W3017797997 cites W2108370954 @default.
• W3017797997 cites W2136808562 @default.
• W3017797997 cites W2146877046 @default.
• W3017797997 cites W2158074397 @default.
• W3017797997 cites W2168570318 @default.
• W3017797997 cites W2194811967 @default.
• W3017797997 cites W2295457071 @default.
• W3017797997 cites W2340722744 @default.
• W3017797997 cites W2396265011 @default.
• W3017797997 cites W2502485013 @default.
• W3017797997 cites W2531862774 @default.
• W3017797997 cites W2585563423 @default.
• W3017797997 cites W2604602378 @default.
• W3017797997 cites W2668893640 @default.
• W3017797997 cites W2763717796 @default.
• W3017797997 cites W2774074688 @default.
• W3017797997 cites W2784429424 @default.
• W3017797997 cites W2790670455 @default.
• W3017797997 cites W2809078763 @default.
• W3017797997 cites W2903065352 @default.
• W3017797997 cites W2913751708 @default.
• W3017797997 cites W2930823845 @default.
• W3017797997 cites W2936955359 @default.
• W3017797997 cites W2940820512 @default.
• W3017797997 cites W2948860485 @default.
• W3017797997 cites W2959655953 @default.
• W3017797997 cites W2967363264 @default.
• W3017797997 cites W2983864784 @default.
• W3017797997 cites W2989725607 @default.
• W3017797997 cites W3010559003 @default.
• W3017797997 cites W3098899160 @default.
• W3017797997 cites W3099001056 @default.
• W3017797997 cites W3099085467 @default.
• W3017797997 cites W3099230470 @default.
• W3017797997 cites W3100504282 @default.
• W3017797997 cites W3100768471 @default.
• W3017797997 cites W3100831909 @default.
• W3017797997 cites W3100991411 @default.
• W3017797997 cites W3102062323 @default.
• W3017797997 cites W3102134091 @default.
• W3017797997 cites W3102191229 @default.
• W3017797997 cites W3102386126 @default.
• W3017797997 cites W3102485047 @default.
• W3017797997 cites W3103693259 @default.
• W3017797997 cites W3104175243 @default.
• W3017797997 cites W3104659524 @default.
• W3017797997 cites W3125416070 @default.
• W3017797997 doi "https://doi.org/10.1093/mnras/staa1037" @default.
• W3017797997 hasPublicationYear "2020" @default.
• W3017797997 type Work @default.
• W3017797997 sameAs 3017797997 @default.
• W3017797997 citedByCount "17" @default.
• W3017797997 countsByYear W30177979972021 @default.
• W3017797997 countsByYear W30177979972022 @default.
• W3017797997 countsByYear W30177979972023 @default.
• W3017797997 crossrefType "journal-article" @default.
• W3017797997 hasAuthorship W3017797997A5014975239 @default.
• W3017797997 hasAuthorship W3017797997A5051918386 @default.
• W3017797997 hasAuthorship W3017797997A5057592704 @default.
• W3017797997 hasBestOaLocation W30177979971 @default.
• W3017797997 hasConcept C10632323 @default.
• W3017797997 hasConcept C121332964 @default.
• W3017797997 hasConcept C125311221 @default.
• W3017797997 hasConcept C127413603 @default.
• W3017797997 hasConcept C1276947 @default.
• W3017797997 hasConcept C14427944 @default.
• W3017797997 hasConcept C146978453 @default.
• W3017797997 hasConcept C150846664 @default.
• W3017797997 hasConcept C163479331 @default.
• W3017797997 hasConcept C17744445 @default.
• W3017797997 hasConcept C178635117 @default.

• next