J/A+A/430/165       Radial velocities for 6691 K and M giants    (Famaey+, 2005)

Local Kinematics of K and M Giants from CORAVEL/Hipparcos/Tycho-2 Data. Revisiting the concept of superclusters. Famaey B., Jorissen A., Luri X., Mayor M., Udry S., Dejonghe H., Turon C. <Astron. Astrophys. 430, 165 (2005)> =2005A&A...430..165F 2005A&A...430..165F
ADC_Keywords: Stars, giant ; Stars, K-type ; Stars, M-type ; Radial velocities ; Space velocities ; Proper motions Keywords: Galaxy: kinematics and dynamics - Galaxy: disk - Galaxy: solar neighbourhood - Galaxy: evolution - Galaxy: structure - stars: kinematics Description: The table provides Hipparcos positions, Hipparcos & Tycho-2 proper motions, and CORAVEL radial velocities for 6691 K and M giants in the solar neighbourhood, mostly from the Hipparcos survey. A bayesian maximum-likelihood approach has been used to derive the distances and space velocities. New V-I indices, computed from a color transformation based on Hp-VT2, are also provided. Spectroscopic binaries have been identified as well. These data may be used to study the kinematics of giant stars in the solar neighbourhood, and to correlate it with their location in the Hertzsprung-Russell diagram. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablea1.dat 312 6690 Catalogue notes.dat 80 19 Individual notes -------------------------------------------------------------------------------- See also: I/239 : The Hipparcos and Tycho Catalogues (ESA 1997) I/259 : The Tycho-2 Catalogue (Hog+ 2000) Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- HIP HIP number (I/239) 8- 13 I6 --- HD HD number (III/135) 16- 23 A8 --- BD BD designation (only when HD missing) 26- 37 F12.8 deg RAdeg Right ascension J2000 (ICRS), Epoch 1991.25, identical to field H8 of Hipparcos Catalogue 39- 50 F12.8 deg DEdeg Declination J2000 (ICRS), Epoch 1991.25, identical to field H9 of Hipparcos Catalogue 53- 59 F7.2 mas varpi Hipparcos parallax 61- 65 F5.2 mas e_varpi Standard error on varpi 69- 74 F6.1 mas/yr pmAT2 Tycho-2 (I/259) proper motion in right ascension, times cos(DE) (1) 76- 79 F4.1 mas/yr e_pmAT2 Standard error on pmAT2 (1) 83- 88 F6.1 mas/yr pmDT2 Tycho-2 proper motion in declination (1) 90- 93 F4.1 mas/yr e_pmDT2 Standard error on pmDT2 (1) 96-102 F7.2 mas/yr pmAH Hipparcos proper motion in right ascension, times cos(RA) 104-108 F5.2 mas/yr e_pmAH Standard error on pmAH 110-117 F8.2 mas/yr pmDH Hipparcos proper motion in declination 119-123 F5.2 mas/yr e_pmDH Standard error on pmDH 125-131 F7.2 --- pmH-T2 Absolute difference between the Hipparcos and Tycho-2 proper motion moduli, normalized by the rms of their standard errors (2) 133-139 F7.4 mag Hpmag Hipparcos Hp magnitude 141-146 F6.4 mag e_Hpmag Standard error on Hp 148-153 F6.3 mag VT2mag Tycho-2 V magnitude 155-160 F6.3 mag Hp-VT2 Difference Hp-V_T2 (3) 162-166 F5.2 mag V-IcH40 Cousins V-I colour index as provided in field H40 of the Hipparcos catalogue 168-172 F5.2 mag V-Ic Cousins V-I colour index, computed from Hp-VT with the colour transformation of Platais et al. (2003, Cat. J/A+A/397/997) 174 A1 --- f_RV [*,0-9] Duplicity flag (4) 177-183 F7.2 km/s RV ? Average radial velocity, or center-of-mass (COM) velocity in the case of a SB (4) 185-189 F5.2 km/s e_RV Standard error of RV 191-195 F5.2 mag MHp Absolute Hp magnitude, based on distance d 197-202 F6.1 pc Dist Maximum-likelihood estimate of the distance 204-209 F6.1 pc e_Dist Standard error on Dist 211-214 F4.2 mag Av Interstellar absorption A_V, estimated for distance Dist with the model of Arenou et al. (1992A&A...258..104A 1992A&A...258..104A) 217-222 F6.1 km/s Uvel U component of the spatial velocity (positive towards the galactic center), based on the distance estimate, and corrected for the galactic differential rotation to first order (using Oort's constants A=14.82km/s/kpc and B=-12.37km/s/kpc) 224-229 F6.1 km/s Vvel V component of the spatial velocity, positive in the direction of galactic rotation 231-236 F6.1 km/s Wvel W component of the spatial velocity, positive towards the north galactic pole 238 I1 --- g [0-6] Kinematic group to which the star has the highest probability to belong (5) 240-244 F5.1 % P(g) Probability (in percent) that the star belongs to group g 246 A1 --- n_HIP [*] note detailed in "notes.dat" file 247-252 F6.3 mag VT2magB ? V_T2 magnitude of the visual companion (when flag B=4) 254-312 A59 --- Ref Bibliographic codes for the orbit used as the source of the COM velocity, separated by comma (6) -------------------------------------------------------------------------------- Note (1): For 291 stars, null values in this and the following three columns indicates that the Tycho-2 is not available or has not been used in the analysis Note (2): Values larger than about 2 hint at the possible binary nature of the star Note (3): For visual binaries (flag = 4 in column B), this colour index has not been listed and a null value is given instead, because the Hp magnitude appears to be a composite value for the two visual components. For large amplitude variable stars, Hp-VT is meaningless as well, and a null value has been listed. Note (4): The duplicity flag has the following meaning: * = no evidence for radial-velocity variations; 0 = spectroscopic binary (SB) with no orbit available; 1 = SB with orbit available (as listed in column Ref), or center-of-mass (COM) velocity can be estimated; Column RV then contains COM velocity; 2 = supergiant (sg) star, with intrinsic radial-velocity noise; 3 = uncertain case: either SB or sg 4 = visual binary with a companion less than 6" apart; 5-8 = as 0-3 but for a component of a visual binary; 9 = binary supergiant with an orbit available The radial velocity contains the center-of-mass velocity for SBs flagged 1 in column f_RV (the last column, Ref, provides then the reference of the orbit used), and standard error (set to 0.3km/s in the case of center-of-mass velocity). For SBs flagged 0 in column 24 (i.e. with no orbit available), average radial velocity and standard error have been put to 0. Note (5): Kinematic groups are numbered as follows: 1 = Y: stars with a young kinematics; 2 = HV: high-velocity stars; 3 = B: smooth background stars; 4 = HyPl: Hyades-Pleiades stream; 5 = Si: Sirius stream; 6 = He: Hercules stream Note (6): The code 2005A&A.in.prep...J refers to the forthcoming paper by Jorissen et al., 2005, devoted to the analysis of the binary content of the present sample. -------------------------------------------------------------------------------- Byte-by-byte Description of file: notes.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- HIP HIP number 8- 80 A73 --- Note Text of Note -------------------------------------------------------------------------------- Acknowledgements: Alain Jorissen, ajorisse(at)astro.ulb.ac.be History: * 04-Oct-2004: Original version * 01-Mar-2005: HIP 58438 = BD+16 2323 instead of BD+34 2323 * 28-Aug-2008: HIP 26247 (RR Cam) removed, was not observed; more details about velocities in binaries added (from Benoit Famaey)
(End) Patricia Vannier [CDS] 04-Oct-2004
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