J/AJ/158/222    Orbits of subsystems in multiple stars. VI.    (Tokovinin, 2019)

Spectroscopic orbits of subsystems in multiple stars. VI. Tokovinin A. <Astron. J., 158, 222 (2019)> =2019AJ....158..222T 2019AJ....158..222T (SIMBAD/NED BibCode)
ADC_Keywords: Stars, double and multiple ; Radial velocities ; Rotational velocities ; Stars, masses Keywords: Binary stars - Multiple stars - Trinary stars Abstract: Thirteen spectroscopic orbits of late-type stars are determined from the high-resolution spectra taken with the CHIRON echelle spectrometer at the 1.5 m Cerro Tololo Inter-American Observatory telescope. Most (HIP 14194B, 40523A, 41171A, 51578A, 57572B, 59426A, 62852B, 66438A, 87813B, and 101472A) are inner subsystems in hierarchical multiple stars with three or four components. The periods range from 2.2 to 1131 days. Masses of the components, orbital inclinations, and projected rotation velocities are estimated, and the presence or absence of the lithium line is noted. In addition to those systems, HIP 57021 is a simple 54 day twin binary, and HIP 111598 is a compact triple-lined system with periods of 5.9 and 271 days. This object is likely old, but, nevertheless, the secondary component in the inner pair does not rotate synchronously with the orbit. The period-eccentricity diagram of 528 known inner low-mass spectroscopic subsystems (including 36 from this paper series) is given. The distribution of the inner periods is smooth, without any details around the tidal circularization period of ∼10 days. Description: The spectra used here were taken with the 1.5 m telescope sited at the Cerro Tololo Inter-American Observatory in Chile and operated by the Small & Moderate Aperture Research Telescope System (SMARTS) Consortium (http://www.astro.yale.edu/smarts/). The observing time (20 hr per semester) was allocated through the National Optical Astronomy Observatory (NOAO). Observations were made with the CHIRON optical echelle spectrograph (Tokovinin et al. 2013PASP..125.1336T 2013PASP..125.1336T) by the telescope operators in service mode. The RVs are determined from the cross-correlation function (CCF) of echelle orders with the binary mask based on the solar spectrum, as detailed in Tokovinin (2016, J/AJ/152/11). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 70 20 Basic parameters of observed multiple systems table2.dat 40 29 Cross-correlation function (CCF) parameters table3.dat 139 13 Spectroscopic orbits table4.dat 45 337 Radial velocities and residuals table5.dat 26 21 Radial velocities of other components -------------------------------------------------------------------------------- See also: B/wds : The Washington Visual Double Star Catalog (Mason+ 2001-2014) I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007) I/345 : Gaia DR2 (Gaia Collaboration, 2018) J/A+A/382/118 : Spectroscopic sub-systems in multiple stars (Tokovinin+, 2002) J/AJ/152/10 : Spectroscopy of subsystems in four multiple stars (Tokovinin, 2016) J/AJ/152/11 : Orbits of four triple stars (Tokovinin, 2016) J/AJ/156/48 : Orbits of subsystems in six multiple stars. III. (Tokovinin, 2018) J/AJ/156/194 : Orbits of double-lined pairs in multiple stars (Tokovinin, 2018) J/ApJS/235/6 : Updated Multiple Star Catalog (MSC); August 2019 (Tokovinin, 2018) J/AJ/157/91 : Radial velocities of subsystems in multiple stars (Tokovinin, 2019) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- WDS WDS identification (HHMMm+DDMM, J2000) 12- 13 A2 --- Comp Component(s) designation 15- 20 I6 --- HIP [14194/111598] Hipparcos number 22- 27 I6 --- HD [18795/214169] HD number 29- 34 A6 --- SpType Spectral type 36- 40 F5.2 mag Vmag [5.63/11.97] V band magnitude 42- 45 F4.2 mag V-K [0.19/2.89]? V-K color index 47- 50 I4 mas/yr pmRA [-279/166] Proper motion in right ascension direction (pmRA*cosDE) (1) 52- 55 I4 mas/yr pmDE [-124/172] Proper motion in declination direction (1) 57- 62 F6.2 km/s RV [-89.87/36.12] Radial velocity 63 A1 --- u_RV [:] Uncertainty flag on RV 65- 69 F5.2 mas Plx [6.17/29.67] Parallax (1) 70 A1 --- n_Plx [b] Note on Plx (2) -------------------------------------------------------------------------------- Note (1): Proper motions and parallaxes are taken from the Gaia DR2 (Gaia Collaboration et al. 2018, Cat. I/345), where available. Note (2): Note as follows: b = Hipparcos parallax (van Leeuwen 2007, Cat. I/311). -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- HIP [14194/111598] Hipparcos number 8- 9 A2 --- Comp Component(s) designation 11- 12 I2 --- N [1/24] Number of averaged measurements 14- 18 F5.3 --- a [0.014/0.522] Dip amplitude 20- 25 F6.3 km/s sigma [3.168/24.05] Dispersion σ of a 27- 31 F5.3 km/s asigma [0.043/2.188] Product aσ proportional to the dip area 33- 36 F4.1 km/s Vsini [0/43] Projected rotation velocity 37 A1 --- u_Vsini [:] Uncertainty flag on Vsini 39- 40 A2 --- Li Presence or absence of the lithium 6708 Å line in individual components -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- HIP [14194/111598] Hipparcos number 8- 12 A5 --- Syst System designation 14- 23 F10.5 d Per [2.19189/1136] Period 25- 31 F7.5 d e_Per [1e-05/5.8] Uncertainty in Per 33- 42 F10.4 d T [53759.4/58560.7] Julian Date (JD-2400000) 44- 49 F6.4 d e_T [0.0007/9.11] Uncertainty in T 51- 56 F6.4 --- e [0/0.575] Eccentricity 58- 63 F6.4 --- e_e [0.0005/0.038]? Uncertainty in e 64 A1 --- f_e [f] f for fixed value 66- 70 F5.1 deg omegaA [0/308.1] Longitude of periastron for the primary component ωA 72- 75 F4.2 deg e_omegaA [0.01/2.1]? Uncertainty in omegaA 76 A1 --- f_omegaA [f] f for fixed 78- 83 F6.3 km/s K1 [10.027/67.484] Radial velocity amplitude of the primary component 85- 90 F6.4 km/s e_K1 [0.0039/0.754] Uncertainty in K1 92- 97 F6.3 km/s K2 [10.241/71.379]? Radial velocity amplitude of the secondary component 99-103 F5.3 km/s e_K2 [0.026/1.874]? Uncertainty in K2 105-111 F7.3 km/s gamma [-89.867/36.121]? Center-of-mass velocity γ 113-117 F5.3 km/s e_gamma [0.01/0.341]? Uncertainty in gamma 119-122 F4.2 km/s rms1 [0.03/1.67]? Weighted rms residual for the primary component 124-127 F4.2 km/s rms2 [0.03/0.37]? Weighted rms residual for the secondary component 129-132 F4.2 Msun M1sin3i [0.27/1.49] Mass of the primary for double-lined system, M1sin3i 133 A1 --- u_M1sin3i [:] Uncertainty flag in M1sin3i 135 A1 --- l_M2sin3i [>] Limit flag on M2sin3i 136-139 F4.2 Msun M2sin3i [0.27/1.28] Mass of the secondary M2sin3i -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- HIP [14194/111598] Hipparcos number 8- 12 A5 --- Syst System designation 14- 23 F10.4 d Date [50301.354/58702.7466] Julian Date (JD-2400000) 25- 31 F7.2 km/s RV [-116.04/94.47] Radial velocity 33- 37 F5.2 km/s e_RV [0.05/20] RV error 39- 43 F5.2 km/s O-C [-9.04/6.14] Residual to orbit 45- 45 A1 --- Comp [abc] Component label (a=primary, b=secondary, c=tertiary) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- HIP [40523/66438] Hipparcos number 7 A1 --- Comp [AB] Component designation 9- 18 F10.4 d Date [58193.7/58699.6] Julian Date (JD-2400000) 20- 25 F6.3 km/s RV [-6.4/30.203] Radial velocity 26 A1 --- u_RV [:] Uncertainty flag on RV -------------------------------------------------------------------------------- History: From electronic version of the journal References: Tokovinin et al. Paper I. 2016AJ....152...11T 2016AJ....152...11T, Cat. J/AJ/152/11 Tokovinin et al. Paper II. 2016AJ....152...10T 2016AJ....152...10T, Cat. J/AJ/152/10 Tokovinin et al. Paper III. 2018AJ....156...48T 2018AJ....156...48T, Cat. J/AJ/156/48 Tokovinin et al. Paper IV. 2018AJ....156..194T 2018AJ....156..194T, Cat. J/AJ/156/194 Tokovinin et al. Paper V. 2019AJ....157...91T 2019AJ....157...91T, Cat. J/AJ/157/91
(End) Prepared by [AAS], Tiphaine Pouvreau [CDS] 22-Jan-2020
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