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Nearby Young Stars Selected by Proper Motion. I. Four New Members of the β Pictoris Moving Group From The Tycho-2 Catalog
DOI: 10.1088/0004-6256/137/3/3632 Bibcode: 2009AJ....137.3632L

Lépine, Sébastien; Simon, Michal

We describe a procedure to identify stars from nearby moving groups and associations out of catalogs of stars with large proper motions. We show that from the mean motion vector of a known or suspected moving group, one can identify additional members of the group based on proper motion data and photometry in the optical and infrared, with minimal…

2009 The Astronomical Journal
Hipparcos 68
Speckle Interferometry at Mount Wilson Observatory: Observations Obtained in 2006-2007 and 35 New Orbits
DOI: 10.1088/0004-6256/138/3/813 Bibcode: 2009AJ....138..813H

Mason, Brian D.; Hartkopf, William I.

Results are presented for 607 speckle interferometric observations of double stars, as well as 222 measures of single stars or unresolved pairs. All data were obtained in 2006 and 2007 at the Mount Wilson Observatory, using the 2.5 m Hooker telescope. Separations range from 0farcs06 to 6farcs31, with a median of 0farcs34. These three observing run…

2009 The Astronomical Journal
Hipparcos 44
Binary Stars with Components of Solar Type: 25 Orbits and System Masses
DOI: 10.1088/0004-6256/138/4/1159 Bibcode: 2009AJ....138.1159D

Docobo, J. A.; Ling, J. F.

Revised orbits and system masses are presented for the following 25 visual double stars: WDS 00593-0040 (A 1902), WDS 00596-0111 (A 1903 AB), WDS 01023+0552 (A 2003), WDS 01049+3649 (A 1515), WDS 01234+5809 (STF 115 AB), WDS 02399+0009 (A 1928), WDS 03310+2937 (A 983), WDS 06573-3530 (I 65), WDS 07043-0303 (A 519), WDS 08267+2432 (A 1746 BC), WDS …

2009 The Astronomical Journal
Hipparcos 18
The Frequency of Warm Debris Disks and Transition Disks in a Complete Sample of Intermediate-Mass Glimpse Stars: Placing Constraints on Disk Lifetimes
DOI: 10.1088/0004-6256/137/2/3329 Bibcode: 2009AJ....137.3329U

Kobulnicky, H. A.; Uzpen, B.; Kinemuchi, K.

The incidence of dusty debris disks around low- and intermediate-mass stars has been investigated numerous times in order to understand the early stages of planet formation. Most notably, the Infrared Astronomical Satellite (IRAS) mission observed the entire sky at mid- and far-infrared (IR) wavelengths, identifying the first debris disk systems, …

2009 The Astronomical Journal
Hipparcos 10