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4“...-luminous, peculiar type Ia supernovae indicate that the Chandrasekhar-limit be significantly larger...”
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5“... collapse to stable dark dwarfs (bound states analogous to white dwarfs) near the Chandrasekhar limit...”
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6by Tom F. Neiser“... by the collapse of an antineutrino star that has exceeded its Chandrasekhar limit. To allow the first neutrino...”
Published 2020-01-01
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8“... the Chandrasekhar limit. For relatively low He-accretion rates carbon ignition occurs in the center, leading to a...”
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10“... the Chandrasekhar limit. KPD 1930+2752 is therefore the first known (non-X-ray source) candidate for a Type Ia...”
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11by Finch Nicolle L., Reindl Nicole, Barstow Martin A., Casewell Sarah L., Geier Stephan, Bertolami Marcelo M. Miller, Taubenberger Stefan“... that Hen 2-428 has a doubledegenerate core whose combined mass significantly exceeds the Chandrasekhar...”
Published 2018-04-01
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12by G. A. Carvalho, R. V. Lobato, P. H. R. S. Moraes, José D. V. Arbañil, E. Otoniel, R. M. Marinho, M. Malheiro“... predict a maximum mass limit for white dwarfs slightly above the Chandrasekhar limit, with larger radii...”
Published 2017-12-01
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13by Sumner Starrfield“... and will eventually reach the Chandrasekhar Limit. This evolution could result in a Supernova Ia (SN Ia) explosion...”
Published 2014-02-01
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14by Starrfield S., Timmes F. X., Iliadis C., Hix W. R., Arnett W. D., Meakin C., Sparks W. M.“... cause the WD to gain or lose mass? If it is gaining mass, can it eventually reach the Chandrasekhar...”
Published 2012-06-01
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17by Giora Shaviv“...The so called Chandrasekhar limiting mass is a a quantum mechanical relativistic effect...”
Published 2013-12-01
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