J/AJ/143/129  Photometric and Spectroscopic observations of BF Dra (Lacy+, 2012)

Absolute properties of the eclipsing binary star BF Draconis. Lacy C.H.S., Torres G., Fekel F.C., Sabby J.A., Claret A. <Astron. J., 143, 129 (2012)> =2012AJ....143..129L 2012AJ....143..129L
ADC_Keywords: Binaries, eclipsing ; Radial velocities ; Photometry, UBV ; Photometry, CCD Keywords: binaries: eclipsing - binaries: spectroscopic - stars: fundamental parameters - stars: individual (BF Dra) Abstract: BF Dra is now known to be an eccentric double-lined F6+F6 binary star with relatively deep (0.7mag) partial eclipses. Previous studies of the system are improved with 7494 differential photometric observations from the URSA WebScope and 9700 from the NFO WebScope, 106 high-resolution spectroscopic observations from the Tennessee State University 2m automatic spectroscopic telescope and the 1m coude-feed spectrometer at Kitt Peak National Observatory, and 31 accurate radial velocities from the CfA. Very accurate (better than 0.6%) masses and radii are determined from analysis of the two new light curves and four radial velocity curves. Theoretical models match the absolute properties of the stars at an age of about 2.72Gyr and [Fe/H]=-0.17, and tidal theory correctly confirms that the orbit should still be eccentric. Our observations of BF Dra constrain the convective core overshooting parameter to be larger than about 0.13Hp. We find, however, that standard tidal theory is unable to match the observed slow rotation rates of the components' surface layers. Description: The spectroscopic observations at the Harvard-Smithsonian Center for Astrophysics (CfA) were carried out with two different spectrographs on the 1.5m Tillinghast reflector at the F. L. Whipple Observatory on Mount Hopkins, AZ. Eighteen spectra were gathered by Torres between 2006 April and 2009 May with a Cassegrain-mounted echelle spectrograph ("Digital Speedometer", DS) at a resolving power of R∼35000. Thirteen additional spectra were collected between 2010 March and 2011 November with the bench-mounted fiber-fed echelle instrument TRES at a resolving power of R∼48000. At Fairborn Observatory from 2010 April through 2011 June, Fekel acquired 44 double-lined spectra with the Tennessee State University (TSU) 2m automatic spectroscopic telescope (AST), a fiber fed echelle spectrograph. The resolution was either 0.24 or 0.4Å. In addition, between 2010 June and 2011 April, Fekel of TSU obtained eight additional double-lined spectra (resolution of 0.21Å) with the KPNO coude feed telescope, coude spectrograph, and a CCD camera. Lacy and Sabby of the University of Arkansas (UofA) obtained additional spectra at the KPNO coude-feed spectrometer from 1989 May to 2011 March. The resolution was 0.3Å. One of the telescopes used to obtain the differential photometry is the URSA WebScope inside a Technical Innovations Robo-Dome. The observatory is located on top of Kimpel Hall on the Fayetteville campus. BF Dra was observed by URSA from 2002 February 8 to 2011 September 26. The other telescope we used is the NFO (New Forest Observatory, NM) WebScope located near Silver City, New Mexico. Observations were made from 2005 March 18 to 2011 September 26. Objects: --------------------------------------------------------------------- RA (2000) DE Designation(s) (Period) --------------------------------------------------------------------- 18 50 59.35 +69 52 57.5 BF Dra = BD+69 1006 (P=11.2110011) --------------------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 70 204 Radial velocities of BF Dra and residuals from the fitted orbit table3.dat 51 76 Times of eclipse of BF Dra and residuals from the ephemeris curve fit table5.dat 25 7494 URSA Webscope (Univ. Arkansas) differential photometry of BF Dra table6.dat 25 9744 NFO (New Forest Observatory, New Mexico) differential photometry of BF Dra refs.dat 92 22 References -------------------------------------------------------------------------------- See also: B/gcvs : General Catalogue of Variable Stars (Samus+ 2007-2012) B/sb9 : 9th Catalogue of Spectroscopic Binary Orbits (Pourbaix+ 2004-2013) I/259 : The Tycho-2 Catalogue (Hog+ 2000) III/249 : Stellar radial velocities bibliographic catalog (Malaroda+, 2006) II/271 : TASS Mark IV patches photometric catalog, version 2 (Droege+, 2007) J/A+A/537/A117 : Velocity curves of SW CMa and HW CMa (Torres+, 2012) J/A+A/546/A61 : Radial velocities for XHIP catalogue (de Bruijne+, 2012) J/AJ/142/185 : Properties of the EB stars HY Vir (Lacy+, 2011) J/other/A+ARV/18.67 : Accurate masses and radii of normal stars (Torres+, 2010) J/other/IBVS/5918 : Minima and maxima of 452 variables (Hubscher+, 2010) J/other/IBVS/5941 : Minima and maxima of 292 variables (Hubscher+, 2010) J/AJ/138/1622 : Absolute properties of LV Her (Torres+, 2009) J/other/IBVS/5830 : Minima and maxima of 292 variables (Hubscher+, 2008) J/A+A/446/785 : Catalogue of eclipsing variables (Malkov+, 2006) J/AJ/130/2838 : Velocity and light curves of RW Lac (Lacy+, 2005) J/AcA/54/207 : Ephemerids of eclipsing binaries (Kreiner, 2004) J/AJ/128/1340 : Properties of the EB star V459 Cas (Lacy+, 2004) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 F10.4 d HJD [4470.35/55872.62] Heliocentric Julian Date; HJD-2400000 12- 17 F6.4 --- Phase Orbital phase 19- 25 F7.2 km/s RV1 [-102/44]? Primary radial velocity 27- 33 F7.2 km/s RV2 [-108/44]? Secondary radial velocity 35- 39 F5.2 km/s O-C1 ? Primary (O-C) residual 41- 45 F5.2 km/s O-C2 ? Secondary (O-C) residual 47- 50 A4 --- Place Place/Source of observation (1) 52- 59 A8 --- Obs Observatory (Fairborn or KPNO) (2) 61- 70 A10 --- Inst Instrument (TRES, CORAVEL, DS or coude feed) (3) -------------------------------------------------------------------------------- Note (1): Place/Source of observation as follows: CfA = Harvard-Smithsonian Center for Astrophysics; TSU = Tennessee State University; UofA = University of Arkansas; IM85 = Imbert (1985A&AS...59..357I 1985A&AS...59..357I). Note (2): KPNO = Kitt Peak National Observatory; Note (3): Instrument as follows: CORAVEL = CORAVEL spectrometer; TRES = Tillinghast Reector Echelle Spectrograph (a bench-mounted fiber-fed echelle instrument); DS = Digital Speedmeter (a Cassegrain-mounted echelle spectrograph); coude feed = coude-feed telescope. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 F6.1 yr Year [1931.8/2011.6] Date of minimum light 9- 19 F11.5 d HJD [26631.3/55779.8] Heliocentric Julian Date; HJD-2400000 21- 27 F7.5 d e_HJD Error on HJD (precision) 29- 33 I5 --- Cycle [-2573/27] Cycle number 35 I1 --- Type [1/2] Eclipse type (1=deeper eclipse) (1) 37- 44 F8.5 d O-C [-0.11955/0.14833] (O-C) residual 46- 48 A3 --- Meth Observational method (pe=photoelectric, pg=photographic or vis=visual) 50- 51 I2 --- Ref Reference (in refs.dat file) -------------------------------------------------------------------------------- Note (1): Eclipses of type 1 are the deeper eclipses when the hotter, less massive component (star B) is being eclipsed by the cooler, more massive component (star A). -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 F7.5 --- Phase Orbital phase 9- 13 F5.3 mag DVmag URSA differential V band magnitude 15- 25 F11.5 d HJD [52314/55831] Heliocentric Julian Date; HJD-2400000 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 F7.5 --- Phase [0/1] Orbital phase 9- 13 F5.3 mag DVmag NFO differential V band magnitude 15- 25 F11.5 d HJD [53447/55831] Heliocentric Julian Date; HJD-2400000 -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- Ref [1/22] Reference number 4- 22 A19 --- BibCode Bibliographic code 24- 40 A17 --- Aut Author's name 42- 92 A51 --- Com Comments -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Sylvain Guehenneux [CDS] 01-Jul-2013
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