J/A+A/587/A51       Overlooked wide companions of nearby F stars  (Scholz, 2016)

Overlooked wide companions of nearby F stars. Scholz R.-D. <Astron. Astrophys. 587, A51 (2016)> =2016A&A...587A..51S 2016A&A...587A..51S (SIMBAD/NED BibCode)
ADC_Keywords: Stars, double and multiple ; Stars, nearby ; Stars, F-type ; Proper motions ; Parallaxes, trigonometric Keywords: proper motions - stars: abundances - binaries: general - stars: low-mass - white dwarfs - solar neighbourhood Abstract: We checked a sample of 545 F stars within 50pc for wide companions using existing near-infrared and optical sky surveys. Description: We checked a sample of 545 F stars within 50pc for wide companions using existing near-infrared and optical sky surveys. Applying the common proper motion (CPM) criterion, we detected wide companion candidates with 6-120arcsec angular separations by visual inspection of multi-epoch finder charts and by searching in proper motion catalogues. Final proper motions were measured by involving positional measurements from up to eleven surveys. Spectral types of red CPM companions were estimated from their absolute J-band magnitudes based on the Hipparcos distances of the primaries. In addition to about 100 known CPM objects, we found 19 new CPM companions and confirmed 31 previously known candidates. A few CPM objects are still considered as candidates according to their level of proper motion agreement. Among the new objects there are nine M0-M4, eight M5-M6, one ∼L3.5 dwarf (HD 3861B), and one white dwarf (WD) (HD 2726B), whereas we confirmed two K, 19 M0-M4, six M5-M6, two early-L dwarfs, and two DA WDs as CPM companions. In a few cases, previous spectral types were available that all agree well with our estimates. Two companions (HD 22879B and HD 49933B) are associated with moderately metal-poor Gaia benchmark stars. One doubtful CPM companion, spectroscopically classified as WD but found to be very bright (J=11.1) by others, should either be a very nearby foreground WD or a different kind of object associated with HD 165670. The main results of this research note, data on new, confirmed, and rejected CPM pairs, are listed in tablea1.dat, tableb1.dat, and tablec1.dat, respectively. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablea1.dat 163 38 New CPM companions of nearby F stars tableb1.dat 163 62 Confirmed CPM companions of nearby F stars tablec1.dat 163 4 Rejected CPM pairs including F stars notes.dat 80 64 Notes -------------------------------------------------------------------------------- See also: B/wds : Washington Visual Double Star Catalog (Mason+ 2001-2014) I/259 : The Tycho-2 Catalogue (Hog+ 2000) I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007) I/322 : UCAC4 Catalogue (Zacharias+, 2012) I/329 : URAT1 Catalog ((Zacharias+ 2015) II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) J/AJ/150/141 : UrHip Proper Motion Catalog (Frouard+, 2015) Byte-by-byte Description of file: tablea1.dat tableb1.dat tablec1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 A11 --- Name HD Name of F star primary or CPM companion (1) 12- 15 A4 --- f_Name Uncertainty flag on Name (2) 17- 25 A9 --- n_Name Notes on name in notes.dat file (2) 27- 37 F11.7 deg RAdeg Right Ascension (J2000, at given Epoch) 39- 49 F11.7 deg DEdeg Declination (J2000, at given Epoch) 51 A1 --- n_pos Note on RA and DE in notes.dat file (3) 53- 60 F8.3 yr Epoch Epoch of RA and DE 62- 66 F5.2 mas Plx ? Parallax of F star primary 68- 72 F5.2 mas e_Plx ? Error of Parallax of F star primary 74- 78 F5.1 arcsec Sep ? Separation of CPM companion 80- 82 I3 deg PA ? Position Angle of CPM companion 84 A1 --- n_Sep Note on Sep and PA, in notes.dat file (3) 86- 91 F6.1 mas/yr pmRA Proper motion in RA*cos(DE) (4) 93- 96 F4.1 mas/yr e_pmRA Error of proper motion in RA*cos(DE) (4) 98-103 F6.1 mas/yr pmDE Proper motion in DE (4) 105-108 F4.1 mas/yr e_pmDE Error of proper motion in DE (4) 110-114 A5 --- n_pmRA Notes on pmRA and pmDE, in notes.dat file (3) 116-126 A11 --- o_Epoch Number of epochs used for pmRA and pmDE (5) 128-133 F6.3 mag Jmag J-band magnitude (6) 135-139 F5.3 mag e_Jmag ? Error of J-band magnitude (6) 141-143 A3 --- n_Jmag Note on J-band magnitude, in notes.dat file (3) 145-153 A9 --- SpType Spectral type 155 A1 --- n_SpType Note on Spectral type, in notes.dat file (3)(7) 157-163 A7 --- Refs References (8) -------------------------------------------------------------------------------- Note (1): The names of the primaries are given as HD numbers and letters A or AB (in case of unresolved binaries). The names of the CPM companions are given as HD numbers and letters B or C-H in agreement with or extending previously known (physical or visual) component designations in the Washington Double Star (WDS) catalogue. In case of tablec1.dat, HD or HIP names are given. Note (2): Possible CPM companions, for which at least one of the proper motion components agreed only to within 3 sigma with that of the primary, are marked with (?). Objects with even larger discrepancies, which were considered as doubtful CPM companions, are marked by (??). Note (3): Notes are given as individual small letters (a-z) and/or digits (1-9), separated by commas. A maximum of five notes separated by commas corresponds to the format A9. If only one note is used, the format is A1. The file notes.dat contains 35 rows, one for each of the letters a-z and digits 1-9. Note (4): Proper motions and their errors derived in this paper are rounded to integer values of mas/yr. Note (5): The 11-digit string o_epochs gives the number of epochs from SSS/APM, 2MASS, DENIS, UCAC4, CMC, SDSS, IPHAS, UKIDSS, WISE, URAT1, and VISTA, which were used in the proper motion determination (of the CPM companion). Note (6): Most J magnitudes and their errors were taken from 2MASS (or DENIS) and rounded to 0.01 mag. Note (7): The spectral types of the mostly red CPM companions derived in this paper are based on the known distances of the primaries and the relation between absolute J magnitude and (early-K to late-L) spectral type from Scholz, Meusinger & Jahreis (2005A&A...442..211S 2005A&A...442..211S, Cat. J/A+A/442/211). The companions of metal-poor primaries were considered as subdwarf candidates. Blue CPM companions were assumed to be white dwarfs. Note (8): Four references are given for: - Position/Epoch, - parallax of the primary (OR angular separation and position angle of the CPM companion, where small epoch differences of <0.3yr were neglected in case of URAT1 data), - proper motion, - spectral type. The four references are given as digits (1-9) or capital letters (S,G, or L), separated by commas. References as follows: 1 = URAT1 (Zacharias et al., 2015AJ....150..101Z 2015AJ....150..101Z, Cat. I/329) 2 = 2MASS (Skrutskie et al., 2006AJ....131.1163S 2006AJ....131.1163S, Cat. VII/233) 3 = Hipparcos (van Leeuwen, 2007A&A...474..653V 2007A&A...474..653V, Cat. Cat. I/311) 4 = UrHip (Frouard et al., 2015AJ....150..141F 2015AJ....150..141F, Cat. J/AJ/150/141) 5 = this paper 6 = UKIDSS GPS (Lucas et al., 2008MNRAS.391..136L 2008MNRAS.391..136L, Cat. II/316) 7 = UKIDSS LAS (Lawrence et al., 2007MNRAS.379.1599L 2007MNRAS.379.1599L, Cat. II/314) 8 = Tycho-2 (Hog et al., 2000A&A...355L..27H 2000A&A...355L..27H, Cat. I/259) 9 = corrected Hipparcos data (Fabricius & Makarov, 2000A&AS..144...45F 2000A&AS..144...45F, Cat. J/A+AS/144/45 S = SIMBAD G = SPM4 (Girard et al., 2011AJ....142...15G 2011AJ....142...15G, Cat. I/320) L = Limoges et al. (2013AJ....145..136L 2013AJ....145..136L, Cat. J/AJ/145/136) -------------------------------------------------------------------------------- Byte-by-byte Description of file: notes.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- Note Note code, letters a-z, digits 1-9 3- 80 A78 --- Text Text of the note -------------------------------------------------------------------------------- Acknowledgements: Ralf D. Scholz, rdscholz(at)aip.de
(End) R.-D. Scholz [AIP], Patricia Vannier [CDS] 03-Feb-2016
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