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Cited by 226

The DOI matches its Crossref record; 2 of the 2 references it cites were found in a registry or an index.

Survival of Planetary Systems

Open access
Ward, William R.·1997·The Astrophysical Journal

Abstract

Gravitational interactions (i.e., disk tides) between a newly formed protoplanet and its precursor disk give rise to a net torque that drains angular momentum from the protoplanet's orbit. As a result, protoplanetary objects suffer orbital decay as the disk attempts to destroy the very system it spawns. Survival of a planetary system may be a rather uncertain outcome, and the fraction of circumstellar disks that produce an extant system could be significantly less than unity. Newly discovered close stellar companions may be circumstantial evidence of such large-scale orbit migrations. A scheme for in situ accretion of such objects is outlined that is consonant with a strong tidal influence.

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Metadata

Authors
Ward, W. R.
Venue
The Astrophysical Journal
Published
1997-06-20
Volume
482
Issue
2
Pages
L211-L214
ISSN
0004-637X (ISSN-L)
OpenAlex
W2023690949
Cited by
226
References
2
FWCI
10.53
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Survival of Planetary Systems. https://app.cochat.ai/papers/10.1086/310701
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Ward, W. R. (1997). Survival of Planetary Systems. The Astrophysical Journal. https://doi.org/10.1086/310701

Data sources

Bibliographic data: Semantic Scholar, OpenAlex, Crossref.

Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.