Tests of in situ formation scenarios for compact multiplanet systems

KC Schlaufman - The Astrophysical Journal, 2014 - iopscience.iop.org
Kepler has identified over 600 multiplanet systems, many of which have several planets with
orbital distances smaller than that of Mercury. Because these systems may be difficult to …

Tests of in situ formation scenarios for compact multiplanet systems

KC Schlaufman - Astrophysical Journal, 2014 - osti.gov
Kepler has identified over 600 multiplanet systems, many of which have several planets with
orbital distances smaller than that of Mercury. Because these systems may be difficult to …

Tests of In-Situ Formation Scenarios for Compact Multiplanet Systems

KC Schlaufman - arXiv preprint arXiv:1402.7075, 2014 - arxiv.org
Kepler has identified over 600 multiplanet systems, many of which have several planets with
orbital distances smaller than that of Mercury--quite different from the Solar System. Because …

TESTS OF IN SITU FORMATION SCENARIOS FOR COMPACT MULTIPLANET SYSTEMS

KC Schlaufman - 2014 - dspace.mit.edu
Kepler has identified over 600 multiplanet systems, many of which have several planets with
orbital distances smaller than that of Mercury. Because these systems may be difficult to …

Tests of in situ Formation Scenarios for Compact Multiplanet Systems

KC Schlaufman - The Astrophysical Journal, 2014 - ui.adsabs.harvard.edu
Kepler has identified over 600 multiplanet systems, many of which have several planets with
orbital distances smaller than that of Mercury. Because these systems may be difficult to …

[引用][C] TESTS OF IN SITU FORMATION SCENARIOS FOR COMPACT MULTIPLANET SYSTEMS

KC Schlaufman - The Astrophysical Journal, 2014 - cir.nii.ac.jp
TESTS OF IN SITU FORMATION SCENARIOS FOR COMPACT MULTIPLANET SYSTEMS |
CiNii Research CiNii 国立情報学研究所 学術情報ナビゲータ[サイニィ] 詳細へ移動 検索フォームへ …

Tests of in situ formation scenarios for compact multiplanet systems

KC Schlaufman - Astrophysical Journal, 2014 - inis.iaea.org
[en] Kepler has identified over 600 multiplanet systems, many of which have several planets
with orbital distances smaller than that of Mercury. Because these systems may be difficult to …