J/MNRAS/400/969  ASAS detached eclipsing binaries parameters (Helminiak+, 2009)

Orbital and physical parameters of eclipsing binaries from the All-Sky Automated Survey catalogue. I. A sample of systems with components' masses between 1 and 2M. Helminiak K.G., Konacki M., Ratajczak M., Muterspaugh M.W. <Mon. Not. R. Astron. Soc., 400, 969-983 (2009)> =2009MNRAS.400..969H 2009MNRAS.400..969H
ADC_Keywords: Binaries, eclipsing ; Radial velocities Keywords: techniques: radial velocities - binaries: eclipsing - binaries: spectroscopic - stars: fundamental parameters Abstract: We derive the absolute physical and orbital parameters for a sample of 18 detached eclipsing binaries from the All-Sky Automated Survey (ASAS) data base based on the available photometry and our own radial velocity (RV) measurements. The RVs are computed using spectra we collected with the 3.9-m Anglo-Australian Telescope (AAT) and its University College London Echelle Spectrograph (UCLES), and the 1.9-m Radcliffe telescope and its Grating Instrument for Radiation Analysis with a Fibre-Fed Echelle (GIRAFFE) at the South African Astronomical Observatory (SAAO). In order to obtain as precise RVs as possible, most of the systems were observed with an iodine cell available at the AAT/UCLES and/or analysed using the two-dimensional cross-correlation technique (TODCOR). The RVs were measured with TODCOR using synthetic template spectra as references. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 128 18 18 DEBs from the ASAS data base and our spectroscopic survey table2.dat 207 18 Absolute orbital and physical parameters from our solutions for the investigated targets with 1σ uncertainties tablea1.dat 77 84 Single, absolute RV measurements for all researched objects -------------------------------------------------------------------------------- See also: II/264 : ASAS Variable Stars in South. hemisphere (Pojmanski+ 2002-05) J/AcA/48/35 : All Sky Automated Survey variable stars (Pojmamski 1998) J/AcA/50/177 : All Sky Automated Survey Catalog (Pojmanski+, 2000) J/MNRAS/395/593 : ASAS chromospherically active eclipsing bin. (Parihar+ 2009) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 A13 --- ASAS ASAS designation (HHMMSS+DDMM.m) 14- 16 A3 --- n_ASAS Note on ASAS (1) 18- 36 A19 --- OName Other name(s) 38- 40 A3 --- Tel Telescope/spectrograph (G1) 42- 44 I3 pc Dist ?=- Heliocentric distance (2) 46- 50 F5.2 mag Vmag V maximum magnitude from ASAS 52- 55 F4.2 mag Jmag 2MASS J magnitude 57- 60 F4.2 mag Hmag 2MASS H magnitude 62- 65 F4.2 mag Kmag 2MASS Ks magnitude 67- 70 A4 --- SpT MK spectral type (3) 72- 74 A3 --- New? [Yes No] If the system was not previously known as an eclipsing or spectroscopic binary before ASAS 76-128 A53 --- Ref Reference if previously known -------------------------------------------------------------------------------- Note (1): Notes as follows: a = Photometry is available from ASAS but the star is not indicated as a variable b = Star has a visual and/or physical companion Note (2): The available distances are based on the Hipparcos parallaxes (Perryman et al., 1997, Cat. I/239), except for V415 Aql (Brancewicz & Dworak, 1980, Cat. II/150). Note (3): The spectral type is based on Teff versus V-K relation for dwarfs by Tokunaga (2000, in Cox A.N., ed., Allens' Astrophysical Quantities, 4th edn. Springer-Verlag, New York, p. 143). -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 A13 --- ASAS ASAS designation (HHMMSS+DDMM.M) 15 A1 --- Sol [tim] Solution 21 A1 --- n_Sol [*] * when spectra were tomographically disentangled 23- 31 F9.6 d Per Period 33- 35 I3 10-6d e_Per rms uncertainty on Per 37- 45 F9.4 d T0 T0(PHOEBE), JD-2450000 (1) 47- 51 F5.4 d e_T0 rms uncertainty on T0 53- 58 F6.2 km/s K1 Radial velocity semi-amplitude of primary 60- 63 F4.2 km/s e_K1 rms uncertainty on K1 65- 70 F6.2 km/s K2 Radial velocity semi-amplitude of secondary 72- 75 F4.2 km/s e_K2 rms uncertainty on K2 77- 83 F7.3 km/s Vg Gamma velocity 85- 88 F4.3 km/s e_Vg rms uncertainty on Vg 90- 95 F6.4 --- q Mass ratio, secondary to primary 97-101 F5.4 --- e_q rms uncertainty on q 103-108 F6.3 solRad a Orbit semi-major axis 110-113 F4.3 solRad e_a rms uncertainty on a 115-120 F6.4 --- e Orbit eccentricity 122-126 F5.4 --- e_e ? rms uncertainty on e 128-132 F5.1 deg omega ?=- Longitude of periastron 134-137 F4.1 deg e_omega ? rms uncertainty in omega 139-143 F5.2 deg i Inclination 145-148 F4.2 deg e_i rms uncertainty on inc 150-155 F6.4 solMass M1 Mass of the primary 157-161 F5.4 solMass e_M1 rms uncertainty on M1 163-168 F6.4 solMass M2 Mass of the secondary 170-174 F5.4 solMass e_M2 rms uncertainty on M2 176-180 F5.3 solRad R1 Radius of the primary 182-185 F4.3 solRad e_R1 rms uncertainty on R1 187-191 F5.3 solRad R2 Radius of the secondary 193-196 F4.3 solRad e_R2 rms uncertainty on R2 198-202 F5.3 --- T2/T1 Temperature ratio, secondary to primary 204-207 F4.3 --- e_T2/T1 rms uncertainty on T2/T1 -------------------------------------------------------------------------------- Note (1): In PHOEBE (see Prsa A. 2006, Univ. Ljubljana), T0 corresponds to the far intersection between the projection of the line of sight through the centre of the ellipse on the orbital plane and the ellipse. -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 A13 --- ASAS ASAS designation (HHMMSS+DDMM.M) 15- 23 F9.4 d BJD Time of observation (BJD-2450000) 25- 32 F8.3 km/s V1 Velocity of the primary 34- 38 F5.3 km/s e_V1 Additional error to the formal RV error for V1 40- 45 F6.3 km/s O-C1 Observed minus calculated for V1 47- 54 F8.3 km/s V2 Velocity of the secondary 56- 60 F5.3 km/s e_V2 Additional error to the formal RV error for V2 62- 67 F6.3 km/s O-C2 Observed minus calculated for V2 69 A1 --- Cal [ti] Velocity calibrator (G2) 71- 73 A3 --- Tel Telescope/instrument (G1) 75- 77 A3 --- n_Tel [tds] tds for tomographically disentangled spectra -------------------------------------------------------------------------------- Global notes: Note (G1): Telescope/spectrograph code as follows: R/G = Radcliffe/GIRAFFE A/U = AAT/UCLES Note (G2): Calibrator as follows: t = ThAr-calibrated spectra i = iodine-calibrated spectra m = mixed -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 19-May-2010
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