FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3101292280> ?p ?o ?g. }

• W3101292280 abstract "&lt;p&gt;&lt;span id=&quot;cch_f1e6c44865c6e3a&quot; class=&quot;_mh6 _wsc&quot;&gt;&lt;span class=&quot;_3oh- _58nk&quot;&gt;The Kepler space telescope collected continuous photometry of several Jovian Trojan asteroids in the Solar System during its K2 mission. We extracted light curves 43 new targets from K2 Campaigns 11-19 using our own photometric package developed for moving objects in the Kepler images which, together with the 56 asteroids from Campaign 6, brings the total sample size up to 99 asteroids. We calculated rotational frequencies and amplitudes for each object and their distributions, and we derived statistics on the binary fraction and possible compositions of these asteroids. We find and excess of very slow rotators (&gt;100 hours) and a possible dichotomy in the period distribution. When compared to other space-based photometric results, we find that the distribution of Hilda rotation periods detected with K2 shows the same possible dichotomy, but the large sample of main-belt asteroids measured with the TESS space telescope does not. &lt;/span&gt;&lt;/span&gt;&lt;/p&gt; &lt;p&gt;&lt;span id=&quot;cch_f1e6c44865c6e3a&quot; class=&quot;_mh6 _wsc&quot;&gt;&lt;span class=&quot;_3oh- _58nk&quot;&gt;The excess of slow rotators corroborates with an outward origin, with synchronized binaries migrating inwareds from the Kuiper belt, and some of them dissociating along the way, creating very slowly rotating single objects. Both a low critical density limit and comparison with strengthless ellipsoid models indicate that none of the objects exceed the density of icy objects, further strengthening an inward migration scenario. &lt;/span&gt;&lt;/span&gt;&lt;span id=&quot;cch_f1e6c44865c6e3a&quot; class=&quot;_mh6 _wsc&quot;&gt;&lt;/span&gt;&lt;/p&gt; &lt;p&gt;&lt;span class=&quot;_mh6 _wsc&quot;&gt;&lt;span class=&quot;_3oh- _58nk&quot;&gt;&lt;span id=&quot;cch_f1e6c44865c6e3a&quot; class=&quot;_mh6 _wsc&quot;&gt;We estimate a binary fraction of at least 21% based on the number of high-amplitude, long-period objects, in agreement with earlier results. Large photometric amplitudes are prevalent over the entire period range, and we cannot fit all objects with a strengtless model in rotational equilibrium.&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;/p&gt; &lt;p&gt;&lt;span id=&quot;cch_f1e6c44865c6e3a&quot; class=&quot;_mh6 _wsc&quot;&gt;&lt;span class=&quot;_3oh- _58nk&quot;&gt;We highlight a few individual objects as well. (99306) 2001 SC101 is the only asteroid observed in to Campaigns, from different sides of the Sun, and we find clear differences in the light curve shape. (13062) Podarkes is the principal body of a proposed small family: we detect a rotation period of 245 hr which puts it into the very slow rotator group. Finally, we present the first continuous light curve of (11351) Leucus, one of the targets of the Lucy spacecraft, and confirm that it also rotates exceedingly slowly, with a period of 445 hr.&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;" @default.
• W3101292280 created "2020-11-23" @default.
• W3101292280 creator A5006824983 @default.
• W3101292280 creator A5017030044 @default.
• W3101292280 creator A5027686516 @default.
• W3101292280 creator A5030224716 @default.
• W3101292280 creator A5079591716 @default.
• W3101292280 date "2020-10-08" @default.
• W3101292280 modified "2023-09-27" @default.
• W3101292280 title "Slow rotators and binary candidates among the Jovian Trojans with K2" @default.
• W3101292280 doi "https://doi.org/10.5194/epsc2020-855" @default.
• W3101292280 hasPublicationYear "2020" @default.
• W3101292280 type Work @default.
• W3101292280 sameAs 3101292280 @default.
• W3101292280 citedByCount "0" @default.
• W3101292280 crossrefType "posted-content" @default.
• W3101292280 hasAuthorship W3101292280A5006824983 @default.
• W3101292280 hasAuthorship W3101292280A5017030044 @default.
• W3101292280 hasAuthorship W3101292280A5027686516 @default.
• W3101292280 hasAuthorship W3101292280A5030224716 @default.
• W3101292280 hasAuthorship W3101292280A5079591716 @default.
• W3101292280 hasConcept C121332964 @default.
• W3101292280 hasConcept C1276947 @default.
• W3101292280 hasConcept C150846664 @default.
• W3101292280 hasConcept C44870925 @default.
• W3101292280 hasConcept C58142911 @default.
• W3101292280 hasConcept C68271606 @default.
• W3101292280 hasConceptScore W3101292280C121332964 @default.
• W3101292280 hasConceptScore W3101292280C1276947 @default.
• W3101292280 hasConceptScore W3101292280C150846664 @default.
• W3101292280 hasConceptScore W3101292280C44870925 @default.
• W3101292280 hasConceptScore W3101292280C58142911 @default.
• W3101292280 hasConceptScore W3101292280C68271606 @default.
• W3101292280 hasLocation W31012922801 @default.
• W3101292280 hasOpenAccess W3101292280 @default.
• W3101292280 hasPrimaryLocation W31012922801 @default.
• W3101292280 hasRelatedWork W11437691 @default.
• W3101292280 hasRelatedWork W11633816 @default.
• W3101292280 hasRelatedWork W13922674 @default.
• W3101292280 hasRelatedWork W14310463 @default.
• W3101292280 hasRelatedWork W21702655 @default.
• W3101292280 hasRelatedWork W21963012 @default.
• W3101292280 hasRelatedWork W27897988 @default.
• W3101292280 hasRelatedWork W28081060 @default.
• W3101292280 hasRelatedWork W39951291 @default.
• W3101292280 hasRelatedWork W5673866 @default.
• W3101292280 isParatext "false" @default.
• W3101292280 isRetracted "false" @default.
• W3101292280 magId "3101292280" @default.
• W3101292280 workType "article" @default.