Diversity of planetary systems in low-mass disks

2014/05/08 by María Paula Ronco, G. C. de Elía, Gonzalo C. de Elía
Physics and Astronomy · #Astro and Planetary Science #Astrobiology #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Gravitational microlensing #Low Mass #Physics #Planet #Planetary mass #Planetary system #Planetesimal #Stars #Stellar, planetary, and galactic studies #Terrestrial planet #astro-ph.EP

paper · pdf · doi:10.1051/0004-6361/201323313

published as A&A 567, A54 (2014) · Accepted for publication in Astronomy and Astrophysics - 13 pages, 11 figures

arxiv created 2014/05/08 · openalex publication_date 2014/05/16 · arxiv updated 2014/09/05 · openalex created_date 2022/10/02 · openalex updated_date 2026/07/31

Abstract

Context. Several studies, observational and theoretical, suggest that planetary systems with only rocky planets are the most common in the Universe.

Citations

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