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J/A+A/521/A12   Radial velocities of nearby late-type stars   (Maldonado+, 2010)

A spectroscopy study of nearby late-type stars, possible members of stellar kinematic groups. Maldonado J., Martinez-Arnaiz R.M., Eiroa C., Montes D., Montesinos B. <Astron. Astrophys. 521, A12 (2010)> =2010A&A...521A..12M
ADC_Keywords: Stars, nearby ; Stars, late-type ; Radial velocities Keywords: stars: late-type - stars: kinematics and dynamics - open clusters and associations: general Abstract: Nearby late-type stars are excellent targets for seeking young objects in stellar associations and moving groups. The origin of these structures is still misunderstood, and lists of moving group members often change with time and also from author to author. Most members of these groups have been identified by means of kinematic criteria, leading to an important contamination of previous lists by old field stars. We attempt to identify unambiguous moving group members among a sample of nearby-late type stars by studying their kinematics, lithium abundance, chromospheric activity, and other age-related properties. Description: File table1 contains the name of the observed stars, coordinates, astrometric data, radial velocities and notes. Parallaxes are taken from van Leeuwen (2007, Cat. I/311) and proper motions from Tycho-2 (2000, Cat. I/259). Radial velocities were derived from high-resolution spectra taken with the FOCES spectrograph at the Calar Alto observatory (Almeria, Spain) and the SARG spectrograph at the Telescopio Nazionale Galileo in La Palma (Canary Islands, Spain). Additional spectra from the public library "S4N" (Allende Prieto et al., 2004, Cat. J/A+A/420/183) were also used. Radial velocities were measured by cross-correlating the spectra of our programme stars with spectra of radial velocity standard stars taken from Barnes et al. (1986PASP...98..223B), Beavers et al. (1979PASP...91..698B), and Udry et al. (1999ASPC..185..383U, 1999ASPC..185..367U). For known spectroscopic binaries the radial velocity of the centre of mass of the system is given. These values are from Pourbaix et al. (Cat. B/sb9/) or Eker et al. (2008, Cat. V/128 ). Previous radial velocities reported in the literature are also given for comparison. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 172 495 Positions, proper motions and radial velocities for the observed stars
See also: B/sb9 : SB9: 9th Cat. of Spectroscopic Binary Orbits (Pourbaix+ 2004-09) V/128 : Chromospherically Active Binaries. Third version (Eker+, 2008) V/117 : Geneva-Copenhagen Survey of Solar neighbourhood (Holmberg+ 2007) I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007) I/259 : The Tycho-2 Catalogue (Hog+ 2000) I/239 : The Hipparcos and Tycho Catalogues (ESA 1997) J/AN/328/889 : Mean Radial Velocities of open clusters (Kharchenko+, 2007) J/ApJS/141/503 : Radial Velocities for 889 late-type stars (Nidever+, 2002) J/ApJS/159/141 : Spectroscopic properties of cool stars. I. (Valenti+, 2005) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 6 I6 --- HIP Hipparcos number (Cat. I/239) 8- 13 I6 --- HD ? HD number 15- 16 I2 h RAh Right Ascension J2000 (hours) 18- 19 I2 min RAm Right Ascension J2000 (minutes) 21- 27 F7.4 s RAs Right Ascension J2000 (seconds) 29 A1 --- DE- Declination J2000 (sign) 30- 31 I2 deg DEd Declination J2000 (degrees) 33- 34 I2 arcmin DEm Declination J2000 (minutes) 36- 41 F6.3 arcsec DEs Declination J2000 (seconds) 43- 48 F6.2 mas Plx Trigonometric parallax (milliarcsec) 50- 54 F5.2 mas e_Plx Standard error in Plx (milliarcsec) 56- 63 F8.2 mas/yr pmRA Proper motion mu_alpha.cos(delta) (milliarcsec per year) 65- 69 F5.2 mas/yr e_pmRA Standard error in pmRA (milliarcsec per year) 71- 78 F8.2 mas/yr pmDE Proper motion mu_delta (milliarcsec per year) 80- 84 F5.2 mas/yr e_pmDE Standard error in pmDE 86- 97 A12 --- Obsrun Observing run identifier (1) 98-104 F7.2 km/s RV ? Radial velocity obtained in this work 106-109 F4.2 km/s e_RV ? Standard error in RV 111-117 F7.2 km/s KH07RV ? Radial velocity from Kharchenko et al. (2007, Cat. J/AN/328/889) 119-123 F5.2 km/s e_KH07RV ? Standard error in KH07RV 125-131 F7.2 km/s NO04RV ? Radial velocity from Nordstrom et al. (2004A&A...418..989N, Cat. V/117) 133-137 F5.2 km/s e_NO04RV ? Standard error in NO04RV 139-144 F6.2 km/s NI02RV ? Radial velocity from Nidever et al. (2002, Cat. J/ApJS/141/503) 146-151 F6.1 km/s VF05RV ? Radial velocity from Valenti & Fischer (2005, Cat. J/ApJS/159/141) 153-172 A20 --- Notes Notes (2)
Note (1): Observing run identifier as follows: 1 = Foces05 2 = Foces06A 3 = Sarg06 4 = Foces06B 5 = Sarg07A 6 = Sarg07B 7 = Foces07 8 = Sarg08 9 = S4N-McD 10 = S4N-La Silla Note (2): Notes use the abbreviations: @ = Star with uncertainty in the parallax over 10 milliarcsec # = Star with known planets CAB = Star included in The 3rd Catalogue of Chromospherically Active Binary Stars (2008, Cat. V/128) RV standard = Radial velocity standard star Spec. Binary = Spectroscopy binary from The 9th catalogue of spectroscopic binaries (B/sb9) or SIMBAD
Acknowledgements: Jesus Maldonado, jesus.maldonado(at)uam.es
(End) Jesus Maldonado [UAM, Spain], Patricia Vannier [CDS] 25-Jun-2010
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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