About: Friends of hot jupiters. IV. Stellar companions beyond 50 au might facilitate giant planet formation, but most are unlikely to cause Kozai-Lidov migration

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About: Friends of hot jupiters. IV. Stellar companions beyond 50 au might facilitate giant planet formation, but most are unlikely to cause Kozai-Lidov migration Goto Sponge NotDistinct Permalink

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scientific article published in the Astrophysical Journal

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rdf:type	Item
description	artículu científicu (ast) wetenschappelijk artikel (nl) наукова стаття, опублікована в серпні 2016 (uk) im August 2016 veröffentlichter wissenschaftlicher Artikel (de) article publié dans la revue scientifique Astrophysical Journal (fr) scientific article published in the Astrophysical Journal (en)
publication date	wds:Q57518476-56AEC589-85EB-43EC-AE1E-15CAFF3B9ED9
publication date	2016-08-03 00:00:00Z (xsd:dateTime)
language of work or name	wds:Q57518476-38BF4F0F-B621-4DAA-AFFF-5D04C006BF1D
language of work or name	English
author name string	wds:Q57518476-3FA5C3E0-FECF-4B37-A308-3BCAC027B72F wds:Q57518476-44AF8746-338A-4082-9D61-7624261DCF95 wds:Q57518476-6F0A21CD-8A20-4DAF-87BD-74E083389146 wds:Q57518476-87FA16E1-5D09-46C2-A08A-3E95A6776AB1 wds:Q57518476-9D184AA4-9AD3-4F29-B690-937A0E676ABC wds:Q57518476-ACA74E5C-245F-4A57-8EB2-4E86D903DDCE wds:Q57518476-D7B8378C-2671-445C-8BEE-1CF2090B2A00 wds:Q57518476-E375958B-EBE0-457A-9EFC-E0BBC631066C
author name string	Ji Wang Timothy D. Morton Justin R. Crepp Philip S. Muirhead Dimitri Mawet John A. Johnson Brad Hansen Marta Bryan
rdfs:label	FRIENDS OF HOT JUPITERS. IV. STELLAR COMPANIONS BEYOND 50 au MIGHT FACILITATE GIANT PLANET FORMATION, BUT MOST ARE UNLIKELY TO CAUSE KOZAI–LIDOV MIGRATION (nl) Friends of hot jupiters. IV. Stellar companions beyond 50 au might facilitate giant planet formation, but most are unlikely to cause Kozai-Lidov migration (en)
skos:prefLabel	FRIENDS OF HOT JUPITERS. IV. STELLAR COMPANIONS BEYOND 50 au MIGHT FACILITATE GIANT PLANET FORMATION, BUT MOST ARE UNLIKELY TO CAUSE KOZAI–LIDOV MIGRATION (nl) Friends of hot jupiters. IV. Stellar companions beyond 50 au might facilitate giant planet formation, but most are unlikely to cause Kozai-Lidov migration (en)
name	FRIENDS OF HOT JUPITERS. IV. STELLAR COMPANIONS BEYOND 50 au MIGHT FACILITATE GIANT PLANET FORMATION, BUT MOST ARE UNLIKELY TO CAUSE KOZAI–LIDOV MIGRATION (nl) Friends of hot jupiters. IV. Stellar companions beyond 50 au might facilitate giant planet formation, but most are unlikely to cause Kozai-Lidov migration (en)
author	wds:Q57518476-09B922DE-6DD9-43CE-BD27-C9521C4FF627 wds:Q57518476-1116A638-02DC-4602-BE75-27C6C79B3999 wds:Q57518476-327011DD-5874-447C-AD05-759E9F6F13FA wds:Q57518476-468dff63-4a77-862a-3e45-299938bb388e wds:Q57518476-C6262DA7-8C21-4E14-A9E4-B092255FDAD3 wds:Q57518476-E755EE21-99EB-4AFA-924F-CAF37C3DDC5B wds:Q57518476-EC95512D-CF46-4EE7-82D3-14C5E90FE492
author	Konstantin Batygin Heather A. Knutson Andrew William Howard Ian Crossfield Sasha Hinkley Philip Muirhead Henry Ngo
title	wds:Q57518476-40355575-9CD4-416F-8906-4FB6864C8E6C
title	Friends of hot jupiters. IV. Stellar companions beyond 50 au might facilitate giant planet formation, but most are unlikely to cause Kozai-Lidov migration (en)
page(s)	wds:Q57518476-CBAF9E7F-871F-4939-A287-A19D42CFBBBA
page(s)	8–8
Internet Archive ID	wds:Q57518476-99D23BF0-FE2F-44EE-873A-779FFE5D301F
Internet Archive ID	arxiv-1606.07102
instance of	wds:Q57518476-F6F1BD85-E8AB-49B2-BE20-AB554625A904
instance of	scholarly article
published in	wds:Q57518476-CF92B684-3267-4BD8-A409-5D44305834F7
full work available at URL	wds:Q57518476-C91F9B1A-78FC-4F44-BFDD-AA26654FB851
published in	The Astrophysical Journal
full work available at URL	https://iopscience.iop.org/article/10.3847/0004-637X/827/1/8/pdf
issue	wds:Q57518476-85256F13-0050-40E8-8754-1298558BCB6E
volume	wds:Q57518476-0013A061-B2CA-479E-9F81-E7F4052FA741
issue	1
volume	827
DOI	wds:Q57518476-A332C35F-EB95-4130-8315-FEF65E235CCC
DOI	http://dx.doi.org/10.3847/0004-637X/827/1/8
DOI	10.3847/0004-637X/827/1/8
arXiv ID	wds:Q57518476-847FFEE2-0F55-4714-9D9A-2064E5B53FAD
arXiv ID	1606.07102
ADS bibcode	wds:Q57518476-9F294433-5DC1-465D-B738-A763B21727B5
ADS bibcode	2016ApJ...827....8N
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q57518476
is cites work of	Brown dwarf companion with a period of 4.6 yr interacting with the hot Jupiter CoRoT-20 b HATS-22b, HATS-23b and HATS-24b: three new transiting super-Jupiters from the HATSouth project WASP-180Ab: Doppler tomography of a hot Jupiter orbiting the primary star in a visual binary Observational evidence for two distinct giant planet populations Eccentricity in planetary systems and the role of binarity Populations of Planets in Multiple Star Systems Detection of the tidal deformation of WASP-103b at 3 σ with CHEOPS Investigating the physical properties of transiting hot Jupiters with the 1.5-m Kuiper Telescope
is cites work of	wds:Q56476079-892D8A4A-FB6E-46B2-9B05-07F5A2AE1698 wds:Q105520152-A2245CFD-86BF-452E-83AB-700D038867DB wds:Q58286250-979E8A69-77B5-4B67-93FA-D8218DA601CE wds:Q60895337-E8D41255-4902-4A99-B6A7-FE3B0AF6B340 wds:Q68491643-93ADAE64-9A65-412A-B12E-E00D615EB3C0 wds:Q112035267-F2CF844A-E30F-4A83-9397-42BB5CB89DA0 wds:Q57852471-272DCE5E-A520-43B2-A8FE-967A6B5E348D wds:Q57444183-CEDC3823-598C-4A4D-BE0F-8B05802CD62E

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