ScholarLens Back to search
2009•IcarusOpen access

Metallicity of the massive protoplanets around HR 8799 If formed by gravitational instability

Ravit Helled, Peter Bodenheimer

Open full text 63 citations

Abstract

This record does not include an abstract. Use the full-text link above if available.

Open-access reader

About this research paper

What this paper is about

An abstract is not available in the OpenAlex record for this paper.

Why it matters

OpenAlex reports 63 citations for this work. Citation counts describe recorded attention and do not establish research quality.

Key contribution

A contribution statement is not available in the OpenAlex record.

Method / approach

Method details are not available in the OpenAlex metadata.

Main findings

Findings are not separately available in the OpenAlex metadata.

Limitations

Limitations are not available in the OpenAlex metadata.

Applications

Application details are not available in the OpenAlex metadata.

Key concepts: Planetesimal, Protoplanet, Physics, Planet, Gas giant, Astronomy, Astrophysics, Accretion (finance)

Related papers

Related paper 1Related paper 2Related paper 3
Back to paper searchBrowse research topicsOriginal source
Metallicity of the massive protoplanets around HR 8799 If formed by gravitational instability — Research Paper | ScholarLens