4 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- American Association of Variable Star ObserversUS2 papers
- Astronomical Institute of the Slovak Academy of SciencesSK2 papers
- Astronomical Observatory of CapodimonteIT2 papers
- Austrian Federal RailwaysAT2 papers
- Bundesdeutsche Arbeitsgemeinschaft für Veränderliche SterneDE2 papers
- Federico Santa María Technical UniversityCL2 papers
- Instituto de Astrofísica de CanariasES2 papers
- National ObservatoryBR2 papers
- Observatori de l'EbreES2 papers
- Silesian University of TechnologyPL2 papers
- Stichting tot Steun VCVGZNL2 papers
- Texas Tech UniversityUS2 papers
3 papers
The evolutionary history of ultra-compact accreting binaries. I. Chemical abundances and formation channel of the eclipsing AM CVn system ZTF J225237.05-051917.4 from HST spectroscopy
W. Yu, A. F. Pala, T. Kupfer +33
AM Canum Venaticorum (AM CVn) stars are ultra-compact binary systems composed of a white dwarf (WD) primary accreting from a H-deficient donor. They are important as potential prog…
The elusive chase for the first RR Lyr star in a binary system: the case of KIC 2831097
Ennio Poretti, Jean-Francois Le Borgne, Mercedes Correa +9
The lack of RR Lyr stars in binary systems is an atypical fact when we compared it to other classes of variables. Therefore, it has become a challenge for observers to detect an RR…
Revisiting the extremely long-period cataclysmic variables V479 Andromedae and V1082 Sagitarii
Gagik Tovmassian, Diogo Belloni, Anna F. Pala +56
The overwhelming majority of CVs have orbital periods shorter than 10 hr. However, a few have much longer periods, and their formation and existence pose challenges for the CV evol…