RT Journal Article
T1 The first confirmed superoutburst of the SU UMa type dwarf nova SDSS J083931.35+282824.0
A1 Shears, Jeremy
A1 Miguel Agustino, Enrique de
A1 Roberts, George
A1 Collins, Donald F.
A1 Myers, Gordon
A1 Campbell, Tut
AB We report unfiltered CCD photometry of the first confirmed superoutburst of the recently discovered dwarf nova, SDSS J083931.35+282824.0 in April 2010. From a quiescence magnitude of ~19.8 it rose to 14.0, an outburst amplitude of at least 5.8 magnitudes. Only the plateau phase of the outburst was observed during which superhumps with peak-to-peak amplitude of up to 0.28 magnitudes were present, confirming this to be an SU UMa type dwarf nova. The mean superhump period was Psh = 0.07836(2) during the first 3 days and this subsequently decreased to 0.07800(3) d. Analysis of the data revealed tentative evidence for an orbital period Porb = 0.07531(25) d. The fractional superhump period excess was ε = 0.039(6), which is consistent with other dwarf novae of similar orbital period.
PB Cornell University
YR 2010
FD 2010
LK https://hdl.handle.net/10272/21761
UL https://hdl.handle.net/10272/21761
LA eng
NO Shears, J., de Miguel, E., Roberts, G., Collins, D. F., Myers, G., & Campbell, T. (2010). The first confirmed superoutburst of the SU UMa type dwarf nova SDSS J083931.35+282824.0 (Version 1). arXiv. https://doi.org/10.48550/ARXIV.1011.5321
DS Repositorio Institucional de la Universidad de Huelva
RD 31 may 2026