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2002•The Astronomical JournalOpen access

A Near-Infrared, Wide-Field, Proper-Motion Search for Brown Dwarfs

J. L. Hinz, Donald W. McCarthy, Doug Simons, Todd J. Henry, J. Davy Kirkpatrick, Patrick McGuire

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Abstract

A common proper-motion survey of M dwarf stars within 8 pc of the Sun reveals no new stellar or brown dwarf companions at wide separations (∼100–1400 AU). This survey tests whether the brown dwarf "desert" extends to large separations around M dwarf stars and further explores the census of the solar neighborhood. The sample includes 66 stars north of -30° and within 8 pc of the Sun. Existing first-epoch images are compared with new J -band images of the same fields an average of 7 yr later to reveal proper-motion companions within a ∼4' radius of the primary star. No new companions are detected to a J -band limiting magnitude of ∼16.5, corresponding to a companion mass of ∼40 Jupiter masses for an assumed age of 5 Gyr at the mean distance of the objects in the survey, 5.8 pc.

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A common proper-motion survey of M dwarf stars within 8 pc of the Sun reveals no new stellar or brown dwarf companions at wide separations (∼100–1400 AU). This survey tests whether the brown dwarf "desert" extends to large separations around M dwarf stars and further explores the census of the solar neighborhood. The sample includes 66 stars north of -30° and within 8 pc of the Sun. Existing first-epoch images are compared with new J -band images of the same fields an average of 7 yr later to reveal proper-motion companions within a ∼4' radius of the primary star. No new companions are detected to a J -band limiting magnitude of ∼16.5, corresponding to a companion mass of ∼40 Jupiter masses for an assumed age of 5 Gyr at the mean distance of the objects in the survey, 5.8 pc.

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Available abstract

A common proper-motion survey of M dwarf stars within 8 pc of the Sun reveals no new stellar or brown dwarf companions at wide separations (∼100–1400 AU). This survey tests whether the brown dwarf "desert" extends to large separations around M dwarf stars and further explores the census of the solar neighborhood. The sample includes 66 stars north of -30° and within 8 pc of the Sun. Existing first-epoch images are compared with new J -band images of the same fields an average of 7 yr later to reveal proper-motion companions within a ∼4' radius of the primary star. No new companions are detected to a J -band limiting magnitude of ∼16.5, corresponding to a companion mass of ∼40 Jupiter masses for an assumed age of 5 Gyr at the mean distance of the objects in the survey, 5.8 pc.

Key concepts: Brown dwarf, Proper motion, Physics, Stars, Astrophysics, Limiting magnitude, Jupiter (rocket family), Astronomy

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