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The β Pictoris Moving Group

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Zuckerman, B., Song, Inseok, Bessell, M. S., Webb, R. A.·2001·The Astrophysical Journal

Abstract

Following the 1983 IRAS detection and subsequent imaging of its extensive dusty circumstellar disk, β Pictoris became the prototypical and most studied example of a potential forming planetary system. Here we report the identification of 17 star systems, each with one or more characteristics indicative of extreme youth, that are moving through space together with β Pic. This diverse set of ~12 million yr old star systems, which includes a ~35 Jupiter mass brown dwarf, and a wide assortment of dusty circumstellar disks, is the comoving, youthful group closest to Earth. Their unique combination of youth and proximity to Earth makes group members—many of which have masses similar to that of the Sun—prime candidates for imaging of warm planets and dusty circumstellar disks with ground- and space-based telescopes.

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Metadata

Authors
Zuckerman, B., Song, I., Bessell, M. S., & Webb, R. A.
Venue
The Astrophysical Journal
Published
2001-11-20
Volume
562
Issue
1
Pages
L87-L90
ISSN
0004-637X (ISSN-L)
OpenAlex
W2001705480
Cited by
448
References
0
FWCI
11.61
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: The β Pictoris Moving Group. https://app.cochat.ai/papers/10.1086/337968
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Zuckerman, B., Song, I., Bessell, M. S., & Webb, R. A. (2001). The β Pictoris Moving Group. The Astrophysical Journal. https://doi.org/10.1086/337968

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