J/A+A/670/A176      B, V and R band polarimetry of AO Cas   (Abdul Qadir+, 2023)

High-precision broadband linear polarimetry of early-type binaries. III. AO Cassiopeiae revisited. Abdul Qadir Y., Berdyugin A.V., Piirola V., Sakanoi T., Kagitan M. <Astron. Astrophys. 670, A176 (2023)> =2023A&A...670A.176A 2023A&A...670A.176A (SIMBAD/NED BibCode)
ADC_Keywords: Binaries, eclipsing ; Polarization ; Optical Keywords: stars: individual: AO Cassiopeiae - polarization - techniques: polarimetric - binaries close - instrumentation: polarimteters - binaries: eclipsing Abstract: The fact that the O-type close binary star system AO∼Cassiopeiae exhibits variable phase-locked linear polarization has been known since the mid-1970s. In this work, we re-observe the polarization arising from this system more than 50 years later to better estimate the interstellar polarization and to independently derive the orbital parameters, such as inclination, i, orientation, Ω, and the direction of the rotation for the inner orbit from the phase-folded polarization curves of the Stokes q and u parameters. The Dipol-2 polarimeter was used to obtain linear polarization measurements of AO Cassiopeiae in the B, V, and R passbands with the T60 remotely controlled telescope at an unprecedented accuracy level of ∼0.003%. We have obtained the first proper quantification of the interstellar polarization in the direction heading towards AO Cas by observing the polarization of three neighboring field stars. We employed a Lomb-Scargle algorithm and detected a clear periodic signal for the orbital period of AO Cas. The standard analytical method based on a two-harmonics Fourier fit was used to obtain the inclination and orientation of the binary orbit. Our polarimetric data exhibited an unambiguous periodic signal at 1.76-days, thus confirming the orbital period of the binary system of 3.52-days. Most of the observed polarization is of interstellar origin. The de-biased values of the orbital inclination are i=63+2-3° and orientation of Ω=29° (209°) ±8°. The direction of the binary system rotation on the plane of the sky is clockwise. Description: We observed AO Cas for a total of 39 nights, from October 26, 2020 until February 01, 2021, with the DiPol-2 polarimeter, attached to the remotely controlled T60 telescope at Haleakala Observatory, Hawaii. DiPol-2 uses two dichroic beam-splitters that split the incident light beam into the B, V, and R passbands, which are simultaneously recorded by three CCD cameras. Objects: ------------------------------------------ RA (2000) DE Designation(s) ------------------------------------------ 00 17 43.06 +51 25 59.1 AO Cas = HR 65 ------------------------------------------ File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file pol.dat 78 39 Polarization data of AO Cas -------------------------------------------------------------------------------- See also: J/A+A/591/A92 : BVR polarimetry of HD 48099 (Berdyugin+, 2016) J/A+A/611/A69 : B,V and R band polarimetry of lambda Tau (Berdyugin+, 2018) Byte-by-byte Description of file: pol.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 F12.4 d JD Julian date 14- 20 F7.4 --- q(B) Stokes q in B-band 22- 27 F6.4 --- u(B) Stokes u in B-band 29- 34 F6.4 --- e_q(B) Error of q(B) and u(B) 36- 42 F7.4 --- q(V) Stokes q in V-band 44- 49 F6.4 --- u(V) Stokes u in V-band 51- 56 F6.4 --- e_q(V) Error of q(V) and u(V) 58- 64 F7.4 --- q(R) Stokes q in R-band 66- 71 F6.4 --- u(R) Stokes u in R-band 73- 78 F6.4 --- e_q(R) Error of q(R) and u(R) -------------------------------------------------------------------------------- Acknowledgements: Yasir Abdul Qadir, yasir.abdulqadir(at)utu.fi References: Berdyugin et al., Paper I 2016A&A...591A..92B 2016A&A...591A..92B, Cat. J/A+A/591/92 Berdyugin et al., Paper II 2018A&A...611A..69B 2018A&A...611A..69B, Cat. J/A+A/611/69
(End) Patricia Vannier [CDS] 23-Jan-2023
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