25 citations · 59 across the 4 of their papers we have counts for
4 papers
The field high-amplitude SX Phe variable BL Cam: results from a multisite photometric campaign. II. Evidence of a binary - possibly triple - system
S. Fauvaud, J. -P. Sareyan, I. Ribas +45
Short-period high-amplitude pulsating stars of Population I ( Sct stars) and II (SX Phe variables) exist in the lower part of the classical (Cepheid) instability strip. Most of…
Toward Understanding The B[e] Phenomenon: III. Properties of the optical counterpart of IRAS 00470+6429
A. S. Miroshnichenko, E. L. Chentsov, V. G. Klochkova +19
FS CMa type stars are a group of Galactic objects with the B[e] phenomenon. They exhibit strong emission-line spectra and infrared excesses, which are most likely due to recently f…
SDSS J080434.20+510349.2: Eclipsing WZ Sge-Type Dwarf Nova with Multiple Rebrightenings
Taichi Kato, Elena P. Pavlenko, Hiroyuki Maehara +8
We observed the 2006 superoutburst of SDSS J080434.20+510349.2 during its plateau phase, rebrightening phase, and post-superoutburst final decline. We found that this object is a g…
Observations of the first confirmed superoutburst of SDSS J080434.20+510349.2 in 2006 March
Jeremy Shears, Geir Klingenberg, Pierre de Ponthiere
During 2006 March the first confirmed superoutburst of the dwarf nova SDSS J080434.20+510349.2 was observed using unfiltered CCD photometry. Time-series photometry revealed superhu…