Plausible explanations for the variations of orbital period in the old nova DQ HerculisDAI, Z. B; QIAN, S. B.Astronomy and astrophysics (Berlin. Print). 2009, Vol 503, Num 3, pp 883-888, issn 0004-6361, 6 p.Article

Orbital period analyses for two cataclysmic variables: UZ Fornacis and V348 Puppis inside the period gapDAI, Z.-B; QIAN, S.-B; FERNANDEZ LAJUS, E et al.Monthly notices of the Royal Astronomical Society (Print). 2010, Vol 409, Num 3, pp 1195-1202, issn 0035-8711, 8 p.Article

Orbital period changes of the nova-like cataclysmic variable AC Cancri : evidence of magnetic braking and an unseen companionQIAN, S.-B; DAI, Z.-B; HE, J.-J et al.Astronomy and astrophysics (Berlin. Print). 2007, Vol 466, Num 2, pp 589-594, issn 0004-6361, 6 p.Article

MAGNETIC BRAKING AND THE EVOLUTION OF THE HW VIR-LIKE BINARY STARSQIAN, S.-B; DAI, Z.-B; ZHU, L.-Y et al.The Astrophysical journal. 2008, Vol 689, Num 1, issn 0004-637X, L49-L52, 2Article

CIRCUMBINARY PLANETS ORBITING THE RAPIDLY PULSATING SUBDWARF B-TYPE BINARY NY VirQIAN, S.-B; ZHU, L.-Y; DAI, Z.-B et al.The Astrophysical journal. 2012, Vol 745, Num 2, issn 0004-637X, L23.1-L23.5, 2Article