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J/AJ/124/1118 Radial velocities of high-velocity white dwarfs (Silvestri+, 2002)
Wide binary systems and the nature of high-velocity white dwarfs. Silvestri N.M., Oswalt T.D., Hawley S.L. <Astron. J. 124, 1118 (2002)> =2002AJ....124.1118S
ADC_Keywords: Stars, double and multiple ; Stars, white dwarf ; Radial velocities Keywords: binaries: general - Galaxy: disk - Galaxy: kinematics and dynamics - stars: fundamental parameters - white dwarfs Description: Radial velocities and complete space motions were measured for 116 white dwarf stars with M dwarf companions (WD+M), including thirteen pairs having "halo-like" velocities. These 116 WD+dM binaries were observed on the 3.5 m telescope at the Apache Point Observatory (APO) on nearly 30 half-nights between 2000 September 4 and 2001 October 20. The APO Double Imaging Spectrograph was used with a 15" slit, yielding a resolution of approximately 2arcsrc/pixel. From the near-solar abundance levels of the M dwarf companions, only one potential stellar halo white dwarf (LP 164-52) was found in the sample, 12 of the 13 high-velocity white dwarfs being actually part of the high-velocity tail of the thick disk rather than the dark matter halo of the Galaxy. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 60 116 116 White Dwarfs in Common Proper Motion Binary Systems
See also: Byte-by-byte Description of file: table1.dat Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 9 A9 --- ID White dwarf identifier assigned by Luyten 11 A1 --- f_ID [b] Note on ID (1) 13- 19 F7.4 h RAh Hour of Right Ascension (B1950) 21- 28 F8.4 deg DEdeg Declination expressed in decimal degrees (B1950) 30- 33 F4.2 arcsec/yr mu Total proper motion 35- 37 I3 deg PAmu Position angle of the total proper motion 39- 43 F5.1 km/s RV Measured radial velocity 45- 48 F4.1 km/s e_RV Error in RV 50- 54 F5.2 mag Vmag The V band magnitude from Smith (1997, Ph.D. thesis, Florida Inst. Technol) 56- 59 F4.1 mag VMag Absolute V band magnitude (2)
Note (1): b: A stellar halo white dwarf candidate. Note (2): Determined from the atmosphere models of Bergeron, Saumon & Wesemael (1995ApJ...443..764B) assuming a log(g)=8.0 WD.
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Bauer [CDS] 26-Nov-2002
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