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....
Combining the spectra obtained at the Palomar 200-inch telescope with the radius estimate from fitting the spectral energy distribution (SED), the visible star was char- acterized to be a hot subdwarf of spectral type OB. The orbital inclination of the system allowed the authors to esti- ...
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 ...
So maybe they have accounting legal issues that dwarf the vast majority of the software houses I do business with. Okay. Yet, no one else manages to ask for a monthly subscription. You could charge each quarter as an option with a reasonable update cost– say, $10, or $25 per app. (...
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 ...
doi:10.1016/j.physrep.2024.05.005Didier SaumonSimon BlouinPier-Emmanuel TremblayElsevier B.V.Physics Reports
Annas, George JMinerva 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, ...
C (2024) 84:698 https://doi.org/10.1140/epjc/s10052-024-13025-9 Regular Article -Theoretical Physics Probing secular changes in the gravitational constant with white dwarf spectra T. D. Le1,2,a 1 Division of Applied Physics, Dong Nai Technology University, Bien Hoa City, Vietnam 2 ...
3 White Dwarf models 3.1 Hydrostatic structure in alternative coupling gravity We model the WD as a static, spherically symmetric star. The star is assumed to be in the hydrostatic equilibrium, which satisfies ∇Φ = − 1 ρ ∇ p. Applying this to Eq. (8), using the EiBI notation,...
Our results also suggest that thousands of years prior to the binary merger, the white dwarf may be heated up significantly by tidal interactions. However, more study is needed since the physical amplitudes of the excited oscillation modes become highly non-linear in the outer layer of the star...