activity
20002016
most citedThe Everchanging Pulsating White Dwarf GD358

66 citations · 374 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.SR2016★ 8 cited

The Magnetic Cataclysmic Variable LSQ1725-64

J. T. Fuchs, Bart H. Dunlap, E. Dennihy +7

We present new photometry and spectroscopy of the 94m eclipsing binary LSQ1725-64 that provide insight into the fundamental parameters and evolutionary state of this system. We con…

astro-ph.SR2013★ 33 cited

Abell 48 - a rare WN-type central star of a planetary nebula

H. Todt, A. Y. Kniazev, V. V. Gvaramadze +18

A considerable fraction of the central stars of planetary nebulae (CSPNe) are hydrogen-deficient. Almost all of these H-deficient central stars (CSs) display spectra with strong ca…

astro-ph.SR2012★ 39 cited

EC 10246-2707: a new eclipsing sdB + M dwarf binary

B. N. Barlow, D. Kilkenny, H. Drechsel +10

We announce the discovery of a new eclipsing hot subdwarf B + M dwarf binary, EC 10246-2707, and present multi-colour photometric and spectroscopic observations of this system. Sim…

astro-ph.SR2012★ 31 cited

Discovery of two new Galactic candidate luminous blue variables with WISE

V. V. Gvaramadze, A. Y. Kniazev, A. S. Miroshnichenko +28

We report the discovery of two new Galactic candidate luminous blue variable (cLBV) stars via detection of circular shells (typical of known confirmed and cLBVs) and follow-up spec…

astro-ph.SR2010★ 27 cited

The absence of sub-minute periodicity in classical T Tauri stars

H. M. Günther, N. Lewandowska, M. P. G. Hundertmark +6

Classical T Tauri stars (CTTS) are young, late-type objects, that still accrete matter from a circumstellar disk. Analytical treatments and numerical simulations predict instabilit…

astro-ph.SR2010★ 21 cited

Multi-site Observations of Pulsation in the Accreting White Dwarf SDSS J161033.64-010223.3 (V386 Ser)

Anjum S. Mukadam, D. M. Townsley, B. T. Gaensicke +20

Nonradial pulsations in the primary white dwarfs of cataclysmic variables can now potentially allow us to explore the stellar interior of these accretors using stellar seismology.…