R. NapiwotzkiCentre of Astrophysics Research, University of Hertfordshire, College Lane, Hatfield AL10 9ABJohn Wiley & Sons, LtdMonthly Notices of the Royal Astronomical SocietyJ. Antoniadis, C. G. Bassa, N. Wex, M. Kramer, and R. Napiwotzki. A white dwarf companion to the relativistic ...
Other cases of white dwarfs with close brown dwarf or stellar companions are explained as the consequence of common-envelope evolution, wherein the original orbit is enveloped during the red giant phase and shrinks owing to friction. In this case, however, the long orbital period (compared with...
Physiological and biochemical characterisation of watered and drought-stressed barley mutants in the HvDWARF gene encoding C6-oxidase involved in brassinosteroid biosynthesis. Plant Physiol. Biochem. 2016, 99, 126–141. [CrossRef] [PubMed] 42. Naser, V.; Shani, E. Auxin response under osmotic ...
In this work, we present the relevant white dwarf cooling limits over the entire A′ mass range. In particular, we have performed a rigorous computation of the luminosities in the resonant regime, where the A′ mass is comparable to the white dwarf plasma frequencies. Keywords: New Gauge ...
The influence of strong, large-scale magnetic fields on the structure and temperature distribution in white dwarf atmospheres is investigated. Magnetic fields may provide an additional component of pressure support, thus possibly inflating the atmosphere compared to the non-magnetic case. Since the ...
Minerva PediatricaANNAS, G. J. -- Health law at the turn of the century : from White Dwarf to Red Giant. Connecticut Law Review. 21 : 3 (1989) 551-569.Annas GJ: Health law at the turn of the century: from white dwarf to red giant. Comm L Rev 2;551- 69, 1989...
As the orbit of the system decays via gravitational radiation, the orbital frequency increases and sweeps through a series of resonances with the g-modes of the white dwarf. At each resonance, the tidal force excites the g-mode to a relatively large amplitude, transferring the orbital energy ...
The two WDs will merge in 37 Myr and most likely form a core He-burning single subdwarf star. J01061000 is the shortest time-scale merger system currently known. The gravitational wave strain from J01061000 is at the detection limit of the Laser Interferometer Space Antenna (LISA). However...
Using this constitutional provision that gives the media the power to serve as one of the...doi:10.1002/scin.5591851106CrockettChristopherJohn Wiley & Sons, Ltd.Science NewsCrockett, C. (2014). White dwarf boosts light of companion. Science News, 185(11), 9-9....
Formation of millisecond pulsars with CO white dwarf companions-I.PSR J1614-2230:evidence for a neutron star born massive. M.Tauris,N.Langer,M.Kramer. Monthly Notices of the Royal Astronomical Society . 2011T. M. Tauris, N. Langer, M. Kramer, Formation of millisecond pulsars with CO white...