most citedHelium Nova on a Very Massive White Dwarf -- A Light Curve Model of V445 Puppis (2000) Revised

67 citations · 199 across the 4 of their papers we have counts for

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astro-ph200867 cited

Helium Nova on a Very Massive White Dwarf -- A Light Curve Model of V445 Puppis (2000) Revised

Mariko Kato, Izumi Hachisu, Seiichiro Kiyota +1

V445 Pup (2000) is a unique object identified as a helium nova. Color indexes during the outburst are consistent with those of free-free emission. We present a free-free emission d…

astro-ph200845 cited

MOST detects SPBe pulsations in HD 127756 & HD 217543: Asteroseismic rotation rates independent of vsini

C. Cameron, H. Saio, R. Kuschnig +7

The MOST (Microvariability and Oscillations of Stars) satellite has discovered SPBe (Slowly Pulsating Be) oscillations in the stars HD 127756 (B1/B2 Vne) and HD 217543 (B3 Vpe). Fo…

astro-ph200824 cited

MOST photometry of the roAp star 10 Aql

D. Huber, H. Saio, M. Gruberbauer +12

Context: We present 31.2 days of nearly continuous MOST photometry of the roAp star 10Aql. Aims:The goal was to provide an unambiguous frequency identification for this little stud…

astro-ph200663 cited

MOST Detects g-Modes in the Late-Type be Star beta CMi (B8Ve)

H. Saio, C. Cameron, R. Kuschnig +10

The Microvariability and Oscillations of stars (MOST) satellite has detected low-amplitude light variations (1 mmag) in the Be star CMi (B8Ve). The observations lasted…

astro-ph200685 cited

Gravity-mode pulsations in subdwarf B stars: a critical test of stellar opacity

C. S. Jeffery, H. Saio

The identification of non-radial g-mode oscillations as the cause of variability in cool subdwarf B stars (PG1716 variables) has been frustrated by a 5 000 K discrepancy between th…

astro-ph2006127 cited

Most Detects G- and P-Modes in the B Supergiant HD 163899 (B2Ib/II)

H. Saio, R. Kuschnig, A. Gautschy +8

The {\it Microvariability and Oscillations of Stars (MOST)} satellite observed the B supergiant HD 163899 (B2 Ib/II) for 37 days as a guide star and detected 48 frequencies $\la$ 2…