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Revista mexicana de astronomía y astrofísica

Print version ISSN 0185-1101

Rev. mex. astron. astrofis vol.49 n.2 Ciudad de México Jan. 2013

 

Articles

 

V1135 Herculis: a double-lined eclipsing binary with an Anomalous Cepheid1

 

E. Sipahi, C. İbanoğlu, Ö. Çakirh, H. A. Dal, and S. Evren

 

Astronomy and Space Sciences Department, Ege University, 35100 Bornova, İzmir, Turkey. (omur.cakirli@gmail.com, ali.dal@mail.ege.edu.tr, serdar@mail.ege.edu.tr, cafer.ibanoglu@mail.ege.edu.tr, esin.sipahi@mail.ege.edu.tr).

 

Received 2013 February 18.
Accepted 2013 April 29.

 

RESUMEN

Se obtuvieron curvas de luz en BVR y velocidades radiales para la binaria eclipsante de doble línea V1135 Her. Nuestro análisis de las curvas de luz en varios colores y de las velocidades radiales nos permitió la determinación de propiedades estelares fundamentales para ambas componentes de este interesante sistema. El sistema está formado por dos estrellas evolucionadas G1+K3, intermedias entre gigantes y supergigantes, con masas M1= 1.461±0.054 M, M2 = 0.504±0.040 M, y radios R1 = 27.1 ±0.4 R, R2 = 10.4±0.2 R. La mayor parte de los parámetros observados y calculados para V1135 Her, así como su ubicación en los diagramas color-magnitud y período-luminosidad indican que su clasificación debe ser Cefeida Anómala.

 

ABSTRACT

BVR light curves and radial velocities for the double-lined eclipsing binary V1135 Her were obtained. Our analyses of the multi-color light curves and radial velocities led to the determination of fundamental stellar properties of both components of the interesting system V1135 Her. The system consists of two evolved stars, G1+K3 between giants and supergiants, with masses of M1 = 1.461 ±0.054 M and M2 = 0.504 ± 0.040 M and radii of R1 = 27.1 ± 0.4 R and R2 = 10.4 ± 0.2 R. Most of the observed and calculated parameters of the VI135 Her and its location on the color-magnitude and period-luminosity diagrams lead to a classification of an Anomalous Cepheid.

Key Words: binaries: close — binaries: eclipsing — binaries: general — binaries: spectroscopic — stars: individual (V1135Her).

 

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Note

1 Based on observations collected at TÜBİTAK National Observatory (Antalya, Turkey).

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