J
J. Bochinski
Researcher at Open University
Publications - 12
Citations - 476
J. Bochinski is an academic researcher from Open University. The author has contributed to research in topics: Exoplanet & White dwarf. The author has an hindex of 9, co-authored 12 publications receiving 420 citations.
Papers
More filters
Journal ArticleDOI
A radio-pulsing white dwarf binary star
T. R. Marsh,Boris T. Gänsicke,Stefan Hümmerich,Franz-Josef Hambsch,Klaus Bernhard,Christopher Lloyd,Elmé Breedt,Elizabeth R. Stanway,Danny Steeghs,Steven G. Parsons,Odette Toloza,Matthias R. Schreiber,Peter G. Jonker,Peter G. Jonker,J. van Roestel,Thomas Kupfer,Anna F. Pala,V. S. Dhillon,V. S. Dhillon,V. S. Dhillon,L. K. Hardy,S. P. Littlefair,A. Aungwerojwit,S. Arjyotha,Detlev Koester,J. Bochinski,Carole A. Haswell,P. Frank,Peter J. Wheatley +28 more
TL;DR: The discovery is reported of a white dwarf/cool star binary that emits from X-ray to radio wavelengths and the spin-down power is an order of magnitude larger than that seen in electromagnetic radiation, which suggests that AR Sco is primarily spin-powered.
Journal ArticleDOI
EL CVn-type binaries - Discovery of 17 helium white dwarf precursors in bright eclipsing binary star systems
Pierre F. L. Maxted,Steven Bloemen,Ulrich Heber,S. Geier,Peter J. Wheatley,T. R. Marsh,Elmé Breedt,D. Sebastian,G. Faillace,Christopher J. Owen,D. Pulley,D. Smith,Ulrich Kolb,Carole A. Haswell,John Southworth,David R. Anderson,Barry Smalley,A. Collier Cameron,Leslie Hebb,E. K. Simpson,Richard G. West,J. Bochinski,R. Busuttil,S. Hadigal,S. Hadigal +24 more
TL;DR: In this article, the authors used the photometric database from the Wide Angle Search for Planets (WASP) to find 17 eclipsing binary stars with orbital periods P = 0.7−2.2 d with similar light curves to 1SWASP J024743.37−251549.2.
Journal ArticleDOI
Direct Evidence for an Evolving Dust Cloud from the Exoplanet KIC 12557548 b
TL;DR: In this paper, the authors present simultaneous multi-color optical photometry using of the transiting exoplanet KIC 12557548 b (also known as KIC1255 b) ULTRACAM.
Journal ArticleDOI
Discovery of WASP-65b and WASP-75b: Two hot Jupiters without highly inflated radii
Y. Gómez Maqueo Chew,Y. Gómez Maqueo Chew,Y. Gómez Maqueo Chew,Francesca Faedi,Don Pollacco,D. J. A. Brown,Amanda P. Doyle,A. Collier Cameron,Michaël Gillon,Monika Lendl,Barry Smalley,Amaury H. M. J. Triaud,Amaury H. M. J. Triaud,Richard G. West,Peter J. Wheatley,R. Busuttil,C. Liebig,David R. Anderson,David J. Armstrong,S. C. C. Barros,J. Bento,J. Bento,J. Bochinski,Vadim Burwitz,Laetitia Delrez,B. Enoch,A. Fumel,Carole A. Haswell,Guillaume Hébrard,Guillaume Hébrard,Coel Hellier,S. Holmes,Emmanuel Jehin,Ulrich Kolb,Pierre F. L. Maxted,James McCormac,Grant Miller,Andrew Norton,Francesco Pepe,Didier Queloz,Didier Queloz,J. E. Rodriguez,Damien Ségransan,Ian Skillen,Keivan G. Stassun,Keivan G. Stassun,Stéphane Udry,Christopher A. Watson +47 more
TL;DR: In this article, the authors reported the discovery of two transiting hot Jupiters, WASP-65b (Mpl = 1.55 ± 0.16 MJ; Rpl =1.11 ± 1.06 RJ), and wasP-75b (mpl = 2.52 ± 2.484 days), which orbit their host star every ∼2.311 days.
Journal ArticleDOI
WASP-54b, WASP-56b and WASP-57b: Three new sub-Jupiter mass planets from SuperWASP ⋆
Francesca Faedi,Francesca Faedi,Don Pollacco,Don Pollacco,S. C. C. Barros,D. J. A. Brown,A. Collier Cameron,Amanda P. Doyle,R. Enoch,Michaël Gillon,Y. Gómez Maqueo Chew,Y. Gómez Maqueo Chew,Y. Gómez Maqueo Chew,Guillaume Hébrard,Guillaume Hébrard,Monika Lendl,C. Liebig,Barry Smalley,Amaury H. M. J. Triaud,Richard G. West,Peter J. Wheatley,Khalid Al-Subai,David R. Anderson,David J. Armstrong,David J. Armstrong,Joao Bento,J. Bochinski,François Bouchy,François Bouchy,R. Busuttil,Luca Fossati,A. Fumel,Carole A. Haswell,Coel Hellier,S. Holmes,Emmanuel Jehin,Ulrich Kolb,James McCormac,James McCormac,Grant Miller,C. Moutou,Andrew Norton,N. R. Parley,Didier Queloz,Alexandre Santerne,Ian Skillen,Alexis M. S. Smith,Stéphane Udry,Christopher A. Watson +48 more
TL;DR: WASP-54b is a sub-Jupiter mass planet of mass 0.636(-0.024)(+0.033)) and radius 1.653 (−0.083)(+ 0.090) R-J as discussed by the authors.