2018 FC4 (French Wikipedia)

Analysis of information sources in references of the Wikipedia article "2018 FC4" in French language version.

refsWebsite
Global rank French rank
485th place
416th place
2nd place
3rd place
75th place
160th place
1,397th place
672nd place
69th place
232nd place
5,591st place
2,911th place
low place
low place
57th place
4th place
low place
low place

aanda.org (Global: 5,591st place; French: 2,911th place)

  • (en) A. A. Christou, N. Georgakarakos, A. Marshall-Lee, A. Humpage, M. ´Cuk, A. Dell’Oro, « New asteroid clusters and evidence of collisional fragmentation in the L5 Trojan cloud of Mars », Astronomy & Astrophysics,‎ (lire en ligne)

arxiv.org (Global: 69th place; French: 232nd place)

dntb.gov.ua (Global: low place; French: low place)

ouci.dntb.gov.ua

  • (en) C de la Fuente Marcos, R de la Fuente Marcos, « Using Mars co-orbitals to estimate the importance of rotation-induced YORP break-up events in Earth co-orbital space », 2021, Monthly Notices of the Royal Astronomical Society, № 4, p. 6007-6025,‎ (lire en ligne)

doi.org (Global: 2nd place; French: 3rd place)

dx.doi.org

  • C de la Fuente Marcos et R de la Fuente Marcos, « Using Mars co-orbitals to estimate the importance of rotation-induced YORP break-up events in Earth co-orbital space », Monthly Notices of the Royal Astronomical Society, vol. 501, no 4,‎ , p. 6007–6025 (ISSN 0035-8711, DOI 10.1093/mnras/stab062, lire en ligne, consulté le ) :

    « Its absolute magnitude is H = 21.3 mag (assumed G = 0.15), which suggests a diameter in the range ∼100–800 m for an assumed albedo in the range 0.60–0.01 (as pointed out above, smaller sizes are far more likely). »

doi.org

  • C de la Fuente Marcos et R de la Fuente Marcos, « Using Mars co-orbitals to estimate the importance of rotation-induced YORP break-up events in Earth co-orbital space », Monthly Notices of the Royal Astronomical Society, vol. 501, no 4,‎ , p. 6007–6025 (ISSN 0035-8711, DOI 10.1093/mnras/stab062, lire en ligne, consulté le ) :

    « Its absolute magnitude is H = 21.3 mag (assumed G = 0.15), which suggests a diameter in the range ∼100–800 m for an assumed albedo in the range 0.60–0.01 (as pointed out above, smaller sizes are far more likely). »

issn.org (Global: 57th place; French: 4th place)

portal.issn.org

  • C de la Fuente Marcos et R de la Fuente Marcos, « Using Mars co-orbitals to estimate the importance of rotation-induced YORP break-up events in Earth co-orbital space », Monthly Notices of the Royal Astronomical Society, vol. 501, no 4,‎ , p. 6007–6025 (ISSN 0035-8711, DOI 10.1093/mnras/stab062, lire en ligne, consulté le ) :

    « Its absolute magnitude is H = 21.3 mag (assumed G = 0.15), which suggests a diameter in the range ∼100–800 m for an assumed albedo in the range 0.60–0.01 (as pointed out above, smaller sizes are far more likely). »

minorplanetcenter.net (Global: 1,397th place; French: 672nd place)

nasa.gov (Global: 75th place; French: 160th place)

ssd.jpl.nasa.gov

oup.com (Global: 485th place; French: 416th place)

academic.oup.com

  • (en) Ying Ding , Yi Qi , Dong Qiao, « Determination method of co-orbital objects in the solar system », Monthly Notices of the Royal Astronomical Society, vol. 526,‎ (lire en ligne)
  • (en) C de la Fuente Marcos, R de la Fuente Marcos, « Using Mars co-orbitals to estimate the importance of rotation-induced YORP break-up events in Earth co-orbital space », Montly Notices, vol. 501,‎ (lire en ligne) :

    « Fig. 2 shows that 2018 FC4 is perhaps the object closest to Eureka in the TMars–λr plane. If future spectroscopic observations provide consistent results, 2018 FC4 could be one of the youngest members of the Eureka family (otherwise, its low TMars relative to Eureka could be mere coincidence). »

scispace.com (Global: low place; French: low place)

  • (en) C. de la Fuente Marcos, R. de la Fuente Marcos, « Using Mars co-orbitals to estimate the importance of rotation-induced YORP break-up events in Earth co-orbital space », Monthly Notices of the Royal Astronomical Society, vol. 501,‎ (lire en ligne) :

    « Our statistical analysis identified three new Mars Trojans: 2009 SE, 2018 EC4, and 2018 FC4. Two of them, 2018 EC4 and 2018 FC4, are probably linked to Eureka but we argue that 2009 SE may have been captured, so it is not related to Eureka. »