J/A+A/404/913 Kinematics and HR Diagrams of Southern Young Stars (Sartori+ 2003)

Formation scenarios for the young stellar associations between galactic longitudes l=280°-360°. Sartori M.J., Lepine J.R.D., Dias W.S. <Astron. Astrophys. 404, 913 (2003)> =2003A&A...404..913S 2003A&A...404..913S
ADC_Keywords: Stars, pre-main sequence ; Stars, early-type ; Positional data ; Proper motions ; Radial velocities ; Space velocities; Photometry; Spectral types ; Extinction ; HR diagrams ; References Keywords: stars: formation - stars: pre-main sequence - stars: early-type - stars: kinematics - Hertzsprung-Russell (HR) and C-M diagrams - open clusters and associations: general Description: We investigate the spatial distribution, the space velocities and age distribution of the pre-main sequence (PMS) stars belonging to Ophiuchus, Lupus and Chamaeleon star-forming regions (SFRs), and of the young early-type star members of the Scorpius-Centaurus (Sco-Cen) OB association. These young stellar associations extend over the galactic longitude range from 280 to 360 degrees, and are at a distance interval of around 100 and 200pc. We present a compilation of PMS and early-type stars members of the investigated SFRs and OB associations. For these lists of stars we give the data used for the study of kinematic properties: positions, adopted distances, proper motions and radial velocities (whenever available), and the basic stellar data, used for the construction of Hertzsprung-Russel diagrams. All data have been taken from the literature. We also present the derived XYZ positions on the Galactic system, UVW components of the space velocities, visual extinction, and bolometric luminosity. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 148 569 Pre-main Sequence Stars table2.dat 194 39 Hipparcos Pre-main Sequence Stars table3.dat 156 520 Early-type stars of the Sco-Cen OB association selected by de Zeeuw et al. (1999AJ....117..354D 1999AJ....117..354D) table4.dat 156 88 Other early-type stars of the Sco-Cen OB association presented by de Geus (1989A&A...216...44D 1989A&A...216...44D) refs.dat 117 62 References -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 20 A20 --- Name Stellar identifier 23- 30 F8.4 deg GLON Galactic longitude 32- 39 F8.4 deg GLAT Galactic latitude 41- 43 A3 --- r_pos Reference for position, in refs.dat file 45- 49 F5.1 mas/yr pmGLON ? Proper motion in galactic longitude (G1) 50- 55 F6.1 mas/yr pmGLAT ? Proper motion in galactic latitude 57- 59 A3 --- r_pm Reference for proper motion, in refs.dat file 61- 65 F5.2 mag Vmag ? Magnitude (apparent) in V filter 67- 70 F4.2 mag V-Ic ? V-I(Cousins) color index 72- 74 A3 --- r_Vmag Reference for V magnitude and (V-Ic), in refs.dat file 76- 84 A9 --- SpType Spectral type 86- 88 A3 --- r_SpType Reference for spectral type, in refs.dat file 90- 93 F4.2 [K] logTeff ? Logarithm of the effective temperature (G2) 95- 97 F3.1 [cm/s2] log(g) ? Logarithm of the superficial gravity (G3) 99-103 F5.2 mag V-Ic_0 ? Intrinsic V-I(Cousins) color index (G4) 105-108 F4.2 mag Av ? Visual Extinction 110-112 I3 pc Dist ? Distance 114 A1 --- r_Dist [abcd] Reference for distance, in refs.dat file 116-120 F5.2 mag BCv ? Bolometric correction in Vmag (G4) 122-126 F5.2 [solLum] log(L) ? Logarithm of the bolometric luminosity 128-144 A17 --- OName Other star identification 146-148 A3 --- Region Star-forming region (1) -------------------------------------------------------------------------------- Note (1): Star-forming region name: Cha = Chamaeleon Lup = Lupus Oph = Ophiuchus -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 20 A20 --- Name Stellar identifier 21- 25 I5 --- HIP Hipparcos number 27 A1 --- Type [CHW?] Type of PMS star (1) 29- 31 A3 --- r_Type Reference for type, in refs.dat file 33- 40 F8.4 deg GLON Galactic longitude (G5) 42- 49 F8.4 deg GLAT Galactic latitude (G5) 51- 56 F6.2 mas Plx Mean trigonometric parallax (G5) 58- 62 F5.2 mas e_Plx Standard error in Plx (G5) 64- 66 I3 pc Dist ? Distance derived from Plx 68- 71 I4 pc E_Dist ? Positive standard error in Dist (2) 74- 76 I3 pc e_Dist ? Negative standard error in Dist (2) 78- 81 I4 pc Xgal ? X position in the Galactic system 83- 86 I4 pc Ygal ? Y position in the Galactic system 88- 91 I4 pc Zgal ? Z position in the Galactic system 93- 98 F6.1 mas/yr pmGLON Proper motion in galactic longitude (G1) 100-105 F6.1 mas/yr pmGLAT Proper motion in galactic latitude 107-111 F5.1 km/s RVel ? Radial velocity 113-115 A3 --- r_RVel ? Reference for RVel, in refs.dat file 117-121 F5.1 km/s Uvel ? U component of space velocity 123-127 F5.1 km/s Vvel ? V component of space velocity 129-133 F5.1 km/s Wvel ? W component of space velocity 135-139 F5.2 mag Vmag ? Magnitude (apparent) in V filter 141-144 F4.2 mag V-Ic ? V-I(Cousins) color index 146-148 A3 --- r_Vmag ? Reference for V magnitude and (V-Ic), in refs.dat file 150-158 A9 --- SpType Spectral type 160-162 A3 --- r_SpType ? Reference for spectral type, in refs.dat file 164-167 F4.2 [K] logTeff ? Logarithm of the effective temperature (G2) 169-171 F3.1 [cm/s2] log(g) ? Logarithm of the superficial gravity (G3) 173-176 F4.2 mag Av ? Visual extinction 178-182 F5.2 [solLum] log(L) ? Logarithm of the bolometric luminosity 184-190 A7 --- OName Other star identification 192-194 A3 --- Region Star-forming region (3) -------------------------------------------------------------------------------- Note (1): Type of PMS star: C = classical T Tauri star H = Herbig Ae/Be star W = weak-line T Tauri star ? = undefined type Note (2): Standard error in Dist was derived from the standard error in Plx Note (3): Star-forming region name: Cen = Centaurus Cha = Chamaeleon Lup = Lupus Oph = Ophiuchus blank = other star-forming regions -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- HD ? HD number 8- 12 I5 --- HIP Hipparcos number 14- 21 F8.4 deg GLON Galactic longitude (G5) 23- 30 F8.4 deg GLAT Galactic latitude (G5) 32- 34 I3 pc Dist Distance derived from Plx 36- 39 I4 pc E_Dist Positive standard error in Dist (1) 42- 44 I3 pc e_Dist Negative standard error in Dist (1) 46- 49 I4 pc Xgal X position on the Galactic system 51- 53 I3 pc Ygal Y position on the Galactic system 55- 58 I4 pc Zgal Z position on the Galactic system 60- 64 F5.1 mas/yr pmGLON Proper motion in galactic longitude (G1) 66- 70 F5.1 mas/yr pmGLAT Proper motion in galactic latitude 72- 76 F5.1 km/s RVel ? Radial velocity 78- 80 A3 --- r_RVel Reference for RVel, in refs.dat file 82- 86 F5.1 km/s Uvel ? U component of space velocity 88- 92 F5.1 km/s Vvel ? V component of space velocity 94- 98 F5.1 km/s Wvel ? W component of space velocity 100-104 F5.2 mag Vmag ? Magnitude (apparent) in V filter (G5) 106-110 F5.2 mag V-Ic ? V-I(Cousins) color index (G5) 112-120 A9 --- SpType Spectral type (G5) 122-125 F4.2 [K] logTeff ? Logarithm of the effective temperature (G2) 127-129 F3.1 [cm/s2] log(g) ? Logarithm of the superficial gravity (G3) 131-135 F5.2 mag V-Ic_0 ? Intrinsic V-I(Cousins) color index (G4) 137-140 F4.2 mag Av ? Visual extinction 142-146 F5.2 mag BCv ? Bolometric correction in Vmag (G4) 148-152 F5.2 [solLum] log(L) ? Logarithm of the bolometric luminosity 154-156 A3 --- Assoc OB Association (2) -------------------------------------------------------------------------------- Note (1): Standard error in Dist was derived from the standard error in Plx Note (2): OB association name: LCC = Lower Centaurus-Crux UCL = Upper Centaurus-Lupus US = Upper-Scorpius -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 A3 --- Ref Reference code 5- 23 A19 --- BibCode BibCode 25- 48 A24 --- Aut Author's name 50-117 A68 --- Com Comments -------------------------------------------------------------------------------- Global notes: Note (G1): Proper motion in galactic longitude is multiplied by the cosine of the galactic latitude Note (G2): Effective temperature was obtained using the relationship between SpType and Teff given by de Jager & Nieuwenhuijzen (1987A&A...177..217D 1987A&A...177..217D) Note (G3): Superficial gravity was derived from SpType and luminosity class as given by Table VII of Straizys & Kuriliene (1981Ap&SS..80..353S 1981Ap&SS..80..353S) Note (G4): These quantities were obtained by interpolation of values in tables 1, 2, 3 or 6 of Bessel et al. (1998A&A...333..231B 1998A&A...333..231B) Note (G5): These quantities were extracted or derived from Hipparcos Catalogue or references therein (ESA, 1997, Cat. I/239) -------------------------------------------------------------------------------- History: * 02-Jul-2003: Original version * 23-Jun-2005: In table4, Positions of HD 120709 to HD 123344 (rec.#37 to 43) corrected Acknowledgments: Marilia Sartori
(End) Patricia Bauer [CDS] 02-Jul-2003
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