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XMM-Newton observations of the low-luminosity cataclysmic variable V405 Pegasi
A. D. Schwope, V. Scipione, I. Traulsen +4
V405 Peg is a low-luminosity cataclysmic variable (CV) that was identified as the optical counterpart of the bright, high-latitude ROSAT all-sky survey source RBS1955. The system w…
Robotic observations of the most eccentric spectroscopic binary in the sky
K. G. Strassmeier, M. Weber, T. Granzer
The visual A component of the Gliese 586AB system is a double-lined spectroscopic binary consisting of two cool stars with the exceptional orbital eccentricity of 0.976. Such an ex…
The PLATO 2.0 Mission
H. Rauer, C. Catala, C. Aerts +159
PLATO 2.0 has recently been selected for ESA's M3 launch opportunity (2022/24). Providing accurate key planet parameters (radius, mass, density and age) in statistical numbers, it…
Long-term photometry of three active red giants in close binary systems: V2253 Oph, IT Com and IS Vir
K. Oláh, A. Moór, K. G. Strassmeier +2
We present and analyze long-term optical photometric measurements of the three active stars V2253 Oph, IT Com and IS Vir. All three systems are single-lined spectroscopic binaries…