2013
DOI: 10.1088/0004-637x/778/2/169
|View full text |Cite
|
Sign up to set email alerts
|

Abstract: The presence of giant gaseous planets that reside in close proximity to their host stars, i.e., hot Jupiters, may be a consequence of large-scale radial migration through the protoplanetary nebulae. Within the framework of this picture, significant orbital obliquities characteristic of a substantial fraction of such planets can be attributed to external torques that perturb the natal disks out of alignment with the spin axes of their host stars. Therefore, the acquisition of orbital obliquity likely exhibits s… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
4
1

Citation Types

3
126
0

Year Published

2014
2014
2019
2019

Publication Types

Select...
3
2
1

Relationship

0
6

Authors

Journals

citations
Cited by 119 publications
(129 citation statements)
references
References 116 publications
3
126
0
Order By: Relevance
“…I), while the rest of the calculation follows directly from Sect. 4 of Batygin & Adams (2013). The results are shown in Fig.…”
Section: Monte Carlo Simulationsmentioning
confidence: 89%
See 4 more Smart Citations
“…I), while the rest of the calculation follows directly from Sect. 4 of Batygin & Adams (2013). The results are shown in Fig.…”
Section: Monte Carlo Simulationsmentioning
confidence: 89%
“…However, within the framework of the picture envisioned by Batygin & Adams (2013), alternative explanations are possible. These include adiabatic trailing of the host star, and early stripping or non-existance of the binary companion.…”
Section: Discussionmentioning
confidence: 99%
See 3 more Smart Citations