Showing 1 - 13 results of 13 for search '"white dwarf"', query time: 0.05s Refine Results
  1. 1
  2. 2
  3. 3
  4. 4

    Effect of Generalized Uncertainty Principle on Main-Sequence Stars and White Dwarfs by Mohamed Moussa

    Published 2015-01-01
    “…Astrophysical objects such as main-sequence stars and white dwarfs are examined and discussed as an application. …”
    Get full text
    Article
  5. 5
  6. 6
  7. 7
  8. 8
  9. 9

    The Unique Helium Nova V445 Puppis Ejected ≫0.001 M⊙ in the Year 2000 and Will Not Become a Type Ia Supernova by Bradley E. Schaefer

    Published 2025-01-01
    “…V445 Puppis (Nova Puppis 2000) is the only known example of a helium nova, where a layer of helium-rich gas accretes onto the surface of a white dwarf (WD) in a cataclysmic variable, with runaway helium burning making for the nova event. …”
    Get full text
    Article
  10. 10

    Hunting for Cold Exoplanets via Microlensing by Beaulieu, Jean-Philippe

    Published 2023-08-01
    “…Microlensing has discovered the first cold super-Earth, and the first Jupiter planet orbiting a white dwarf. It also detected a number of Earth, Super-Earth, Neptune, Saturn, Jupiter, super-Jupiter orbiting main sequence stars in the mass range 0.08 – 1M$\odot $. …”
    Get full text
    Article
  11. 11

    A Multiwavelength Light-curve Analysis of the Classical Nova KT Eri: Optical Contribution from a Large Irradiated Accretion Disk by Izumi Hachisu, Mariko Kato, Frederick M. Walter

    Published 2025-01-01
    “…This result is consistent with the temporal variation of wide-band V brightness that varies almost with the intermediate-band Strömgren y brightness, because the V flux is dominated by continuum radiation, the origin of which is a photospheric emission from the very bright disk. We determined the white dwarf mass to be M _WD = 1.3 ± 0.02 M _⊙ , the hydrogen-burning turnoff epoch to be ∼240 days after the outburst, the distance modulus in the V band to be ( m − M ) _V = 13.4 ± 0.2, and the distance to KT Eri to be d = 4.2 ± 0.4 kpc for the reddening of E ( B − V ) = 0.08. …”
    Get full text
    Article
  12. 12
  13. 13

    Distinguishing Compact Objects in Extreme-Mass-Ratio Inspirals by Gravitational Waves by Lujia Xu, Shucheng Yang, Wenbiao Han, Xingyu Zhong, Rundong Tang, Yuanhao Zhang

    Published 2025-01-01
    “…Therefore, our findings suggest that it is possible to distinguish primordial black holes from white dwarfs, and, under certain conditions, neutron stars can also be differentiated from primordial black holes.…”
    Get full text
    Article