
arXiv: 1804.02360
handle: 21.11116/0000-0005-CE84-E , 20.500.11850/264421
Monthly Notices of the Royal Astronomical Society, 477 (4)
ISSN:0035-8711
ISSN:1365-2966
Earth and Planetary Astrophysics (astro-ph.EP), Accretion, protoplanetary discs; Accretion, accretion discs; planet-disc interactions, Protoplanetary discs, FOS: Physical sciences, Astronomy and Astrophysics, planet-disc interactions, Astrophysics - Astrophysics of Galaxies, protoplanetary discs, Astrophysics - Solar and Stellar Astrophysics, Accretion, accretion discs, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Planet-disc interactions, Accretion discs, Solar and Stellar Astrophysics (astro-ph.SR), Astrophysics - Earth and Planetary Astrophysics
Earth and Planetary Astrophysics (astro-ph.EP), Accretion, protoplanetary discs; Accretion, accretion discs; planet-disc interactions, Protoplanetary discs, FOS: Physical sciences, Astronomy and Astrophysics, planet-disc interactions, Astrophysics - Astrophysics of Galaxies, protoplanetary discs, Astrophysics - Solar and Stellar Astrophysics, Accretion, accretion discs, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Planet-disc interactions, Accretion discs, Solar and Stellar Astrophysics (astro-ph.SR), Astrophysics - Earth and Planetary Astrophysics
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 83 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Top 1% | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Top 10% | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Top 1% |
