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  1. 1
    Quasi-stars and the Schönberg–Chandrasekhar limit
    by Ball, Warrick Heinz
    Published 2012
    “... of the models leads to an extension of the classical Schönberg–Chandrasekhar limit and an exploration...”
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  2. 2
    Dedução do limite de Chandrasekhar: uma abordagem didática dos trabalhos originais do autor
    Subjects: “...Chandrasekhar Limit...”
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    Article
  3. 3
    A Short History of the Discovery of Black Holes
    by Braddock Martin
    Published 2021-02-01
    Subjects: “...chandrasekhar limit...”
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    Article
  4. 4
    Existence of Chandrasekhar’s limit in generalized uncertainty white dwarfs
    by Arun Mathew, Malay K. Nandy
    Published 2021-06-01
    Subjects: “...Chandrasekhar limit...”
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    Article
  5. 5
    Variable G versus the Accelerated Expansion of the Universe
    by Colenbrander Bernard G., Hulscher Willem S.
    Published 2017-12-01
    Subjects: “...chandrasekhar limit...”
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    Article
  6. 6
    Establishing Super- and Sub-Chandrasekar Limiting Mass White Dwarfs to Explain Peculiar Type La Supernovae
    by Das, Upasana
    Published 2018
    Subjects: “...Chandrasekhar Limit...”
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  7. 7
    Dense Stars with Weak Magnetic Fields
    by CHIN-WEN CHEN, 陳錦文
    Published 2001
    “... use the numerical integration method to obtain the Chandrasekhar limit of the dense stars...”
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  8. 8
    Effect of dynamical noncommutativity on the limiting mass of white dwarfs
    by Sayan Kumar Pal, Partha Nandi
    Published 2019-10-01
    “...-luminous, peculiar type Ia supernovae indicate that the Chandrasekhar-limit be significantly larger...”
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    Article
  9. 9
    Slowly-rotating Strange Quark Stars
    by Ming-Che Chang, 張敏哲
    Published 2001
    “... differential equations. Through the numerical analysis we compare the different Chandrasekhar limits between...”
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  10. 10
    Dark Matter as dark dwarfs and other macroscopic objects: multiverse relics?
    “... collapse to stable dark dwarfs (bound states analogous to white dwarfs) near the Chandrasekhar limit...”
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    Article
  11. 11
    Fermi Degenerate Antineutrino Star Model of Dark Energy
    by Tom F. Neiser
    Published 2020-01-01
    “... by the collapse of an antineutrino star that has exceeded its Chandrasekhar limit. To allow the first neutrino...”
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    Article
  12. 12
    Two populations of X-ray pulsars produced by two types of supernovae
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    Article
  13. 13
    The WD+He star binaries as the progenitors of type Ia supernovae
    by Wang Bo, Liu Dongdong
    Published 2017-12-01
    “... the Chandrasekhar limit. For relatively low He-accretion rates carbon ignition occurs in the center, leading to a...”
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    Article
  14. 14
    Probing Post-Explosion Evolution of Supernovae in the Type Ia Single Degenerate Channel
    “... the Chandrasekhar limit (M ∼ 1.4 solar masses). At this point a deflagration wave begins in the core...”
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  15. 15
    The Study of the Highly Compact Stellar Structure
    by Lu, Jing-Yu, 盧勁羽
    Published 1997
    “..., which is 1.4 times the solar mass. This limit is called the Chandrasekhar limit...”
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  16. 16
    A Target or the Next XCov23 Campaign: KPD 1930+2752
    by Charpinet S., Reed M.D.
    Published 2003-03-01
    “... the Chandrasekhar limit. KPD 1930+2752 is therefore the first known (non-X-ray source) candidate for a Type Ia...”
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    Article
  17. 17
    Spectral analysis of the binary nucleus of the planetary nebula Hen 2-428 – first results
    “... that Hen 2-428 has a doubledegenerate core whose combined mass significantly exceeds the Chandrasekhar...”
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    Article
  18. 18
    Stellar equilibrium configurations of white dwarfs in the f(R, T) gravity
    “... predict a maximum mass limit for white dwarfs slightly above the Chandrasekhar limit, with larger radii...”
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    Article
  19. 19
    The accretion of solar material onto white dwarfs: No mixing with core material implies that the mass of the white dwarf is increasing
    by Sumner Starrfield
    Published 2014-02-01
    “... and will eventually reach the Chandrasekhar Limit. This evolution could result in a Supernova Ia (SN Ia) explosion...”
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    Article
  20. 20
    Hydrodynamic Studies of the Evolution of Recurrent, Symbiotic and Dwarf Novae: the White Dwarf Components are Growing in Mass
    “... cause the WD to gain or lose mass? If it is gaining mass, can it eventually reach the Chandrasekhar...”
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    Article
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