Orbit determination for the binary Cepheid V1344 Aql^⋆

¹ HUN-REN Research Centre for Astronomy and Earth Sciences, Konkoly Observatory, Konkoly Thege Miklósút 15-17, Budapest 1121, Hungary
e-mail: cseh.borbala@csfk.hun-ren.hu
² CSFK, MTA Centre of Excellence, Konkoly Thege Miklósút 15-17, Budapest 1121, Hungary
³ MTA-ELTE Lendület “Momentum” Milky Way Research Group, Szent Imre H. str. 112, 9700 Szombathely, Hungary
⁴ Max-Planck-Institute for Astrophysics, Karl-Schwarzschild-Str. 1, 85741 Garching, Germany
⁵ Technical University Munich, TUM Department of Physics, James-Franck-Str. 1, 85741 Garching, Germany
⁶ ELTE Eötvös Loránd University, Gothard Astrophysical Observatory, Szent Imre H. str. 112, 9700 Szombathely, Hungary
⁷ MTA-ELTE Exoplanet Research Group, Szent Imre H. str. 112, 9700 Szombathely, Hungary

Received: 4 July 2023
Accepted: 12 October 2023

Abstract

Context. Binary Cepheids play an important role in the investigation of the calibration of the classical Cepheid period-luminosity relationship. Therefore, a thorough study of individual Cepheids belonging to binary systems is necessary.

Aims. Our aim is to determine the orbit of the binary system V1344 Aql using newly observed and earlier published spectroscopic and photometric data.

Methods. We collected new radial velocity observations using medium resolution (R ≈ 11 000 and R ⪅ 20 000) spectrographs, and we updated the pulsation period of the Cepheid based on available photometric observations using an O − C diagram. Separating the pulsational and orbital radial velocity variations for each observational season (year), we determined the orbital solution for the system using χ² minimisation.

Results. The updated pulsation period of the Cepheid estimated for the epoch of HJD 2458955.83 is 7.476826 days. We determined orbital elements for the first time in the literature. The orbital period of the system is about 34.6 yr, with an eccentricity of e = 0.22.