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R. Helled

38 papers hereh-index 171.1k citations48 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author5
  • middle author14
  • last author18

Across the 37 of 38 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP36
  • astro-ph.IM2
same name
  • R. Helled — 151 papers, h 48
  • R. Helled — 16 papers, h 2
  • R. Helled — 2 papers, h 2

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20182026
most citedForming Mercury by Giant Impacts

85 citations · 717 across the 35 of their papers we have counts for

collaborators
Showing 2018Show all

4 papers · 1 filter

astro-ph.EP2018★ 37 cited

The distribution of heavy-elements in giant protoplanetary atmospheres: the importance of planetesimal-envelope interactions

Claudio Valletta, Ravit Helled

In the standard model for giant planet formation, the planetary growth begins with accretion of solids followed by a buildup of a gaseous atmosphere as more solids are accreted, an…

astro-ph.EP2018★ 12 cited

A Quantitative Comparison of Exoplanet Catalogs

Dolev Bashi, Ravit Helled, Shay Zucker

In this study, we investigated the differences between four commonly-used exoplanet catalogs (exoplanet.eu; exoplanetarchive.ipac.caltech.edu; openexoplanetcatalogue.com; exoplanet…

astro-ph.EP2018★ 85 cited

Forming Mercury by Giant Impacts

Alice Chau, Christian Reinhardt, Ravit Helled +1

The origin of Mercury's high iron-to-rock ratio is still unknown. In this work we investigate Mercury's formation via giant impacts and consider the possibilities of a single giant…

astro-ph.EP2018★ 31 cited

On the diversity in mass and orbital radius of giant planets formed via disk instability

Simon Müller, Ravit Helled, Lucio Mayer

We present a semi-analytical population synthesis model of protoplanetary clumps formed by disk instability at radial distances of 80 - 120 AU. Various clump density profiles, init…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.