Volume 390, Issue 4 pp. 1635-1646

Post-common envelope binaries from SDSS – III. Seven new orbital periods

A. Rebassa-Mansergas

Corresponding Author

A. Rebassa-Mansergas

Department of Physics, University of Warwick, Coventry CV4 7AL

E-mail: [email protected]Search for more papers by this author
B. T. Gänsicke

B. T. Gänsicke

Department of Physics, University of Warwick, Coventry CV4 7AL

Search for more papers by this author
M. R. Schreiber

M. R. Schreiber

Departamento de Física y Astronomía, Universidad de Valparaíso, Avenida Gran Bretana 1111, Valparaíso, Chile

Search for more papers by this author
J. Southworth

J. Southworth

Department of Physics, University of Warwick, Coventry CV4 7AL

Search for more papers by this author
A. D. Schwope

A. D. Schwope

Astrophysikalisches Inst. Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany

Search for more papers by this author
A. Nebot Gomez-Moran

A. Nebot Gomez-Moran

Astrophysikalisches Inst. Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany

Search for more papers by this author
A. Aungwerojwit

A. Aungwerojwit

Department of Physics, University of Warwick, Coventry CV4 7AL

Department of Physics, Faculty of Science, Naresuan University, Phitsanulok 65000, Thailand

Search for more papers by this author
P. Rodríguez-Gil

P. Rodríguez-Gil

Isaac Newton Group of Telescopes, Apdo. de Correos 321, E-38700, Santa Cruz de La Palma, Spain

Instituto de Astrofísica de Canarias, Vía Láctea, s/n, La Laguna, E-38205 Tenerife, Spain

Search for more papers by this author
V. Karamanavis

V. Karamanavis

Department of Physics, Section of Astrophysics, Astronomy & Mechanics, University of Thessaloniki, 541 24 Thessaloniki, Greece

Search for more papers by this author
M. Krumpe

M. Krumpe

Astrophysikalisches Inst. Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany

Search for more papers by this author
E. Tremou

E. Tremou

Department of Physics, Section of Astrophysics, Astronomy & Mechanics, University of Thessaloniki, 541 24 Thessaloniki, Greece

Search for more papers by this author
R. Schwarz

R. Schwarz

Astrophysikalisches Inst. Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany

Search for more papers by this author
A. Staude

A. Staude

Astrophysikalisches Inst. Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany

Search for more papers by this author
J. Vogel

J. Vogel

Astrophysikalisches Inst. Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany

Search for more papers by this author
First published: 27 October 2008
Citations: 10

ABSTRACT

We present follow-up spectroscopy and photometry of 11 post-common envelope binary (PCEB) candidates identified from multiple Sloan Digital Sky Survey (SDSS) spectroscopy in an earlier paper. Radial velocity measurements using the Na iλλ8183.27, 8194.81 absorption doublet were performed for nine of these systems and provided measurements of six orbital periods in the range Porb= 2.7– 17.4 h. Three PCEB candidates did not show significant radial velocity variations in the follow-up data, and we discuss the implications for the use of SDSS spectroscopy alone to identify PCEBs. Differential photometry confirmed one of our spectroscopic orbital periods and provided one additional Porb measurement. Binary parameters are estimated for the seven objects for which we have measured the orbital period and the radial velocity amplitude of the low-mass companion star, Ksec. So far, we have published nine SDSS PCEBs orbital periods, all of them Porb < 1 d. We perform Monte Carlo simulations and show that 3σ SDSS radial velocity variations should still be detectable for systems in the orbital period range of Porb∼ 1– 10 d. Consequently, our results suggest that the number of PCEBs decreases considerably for Porb > 1 d, and that during the CE phase the orbital energy of the binary star is may be less efficiently used to expel the envelope than frequently assumed.

The full text of this article hosted at iucr.org is unavailable due to technical difficulties.