Brian D. Mason et al. 1999 The Astronomical Journal 117 1890 doi:10.1086/300823
Brian D. Mason1,5,6,7,8,9, Christian Martin2,6, William I. Hartkopf2,6,7,8,9, Donald J. Barry3,5,8,9, Marvin E. Germain4,5, Geoffrey G. Douglass4, Charles E. Worley4,10, Gary L. Wycoff4, Theo ten Brummelaar5,6,9 and Otto G. Franz4,5,8,9
Show affiliationsThe ESA Hipparcos satellite made measurements of over 12,000 double stars and discovered 3406 new systems. In addition to these, 4706 entries in the Hipparcos Catalogue correspond to double star solutions that did not provide the classical parameters of separation and position angle (ρ, θ) but were the so-called problem stars, flagged "G," "O," "V," or "X" (field H59 of the main catalog). An additional subset of 6981 entries were treated as single objects but classified by Hipparcos as "suspected nonsingle" (flag "S" in field H61), thus yielding a total of 11,687 "problem stars." Of the many ground-based techniques for the study of double stars, probably the one with the greatest potential for exploration of these new and problem Hipparcos binaries is speckle interferometry. Results are presented from an inspection of 848 new and problem Hipparcos binaries, using both archival and new speckle observations obtained with the USNO and CHARA speckle cameras.
Issue 4 (1999 April)
Received 1998 December 16, accepted for publication 1999 January 12
Brian D. Mason et al. 1999 The Astronomical Journal 117 1890
Fronefield Crawford et al. 2000 The Astronomical Journal 119 2376
Vayujeet Gokhale et al. 2007 ApJ 655 1010
Steve Heathcote et al. 1998 The Astronomical Journal 116 1940
C. Ma et al. 1998 The Astronomical Journal 116 516
Gerald Kaiser 2004 J. Phys. A: Math. Gen. 37 7163
C J Wilson et al 2009 Semicond. Sci. Technol. 24 115018
Robert W Keyes 2005 Rep. Prog. Phys. 68 2701
due to Coulomb focusing in fast proton - neon collisions
Gy Víkor et al 1996 J. Phys. B: At. Mol. Opt. Phys. 29 L787
and
L Zarkova and P Pirgov 1996 J. Phys. B: At. Mol. Opt. Phys. 29 4411