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Autor:
Das, Mayusree, Mukhopadhyay, Banibrata
The existence of massive white dwarfs (WDs) containing more than Chandrasekhar's maximum mass has been suggested via the detection of peculiar type Ia Supernovae. It had been crucial to directly detect those 'super' (more massive)-Chandrasekhar WDs t
Externí odkaz:
http://arxiv.org/abs/2411.19059
Autor:
Das, Mayusree, Mukhopadhyay, Banibrata
In the past decades, several neutron stars (NSs), particularly pulsars, with mass $M>2M_\odot$ have been observed. On the other hand, the existence of massive white dwarfs (WDs), even violating Chandrasekhar mass-limit, was inferred from the peak lum
Externí odkaz:
http://arxiv.org/abs/2302.03706
Autor:
Das, Mayusree1 (AUTHOR) mayusreedas@iisc.ac.in, Mukhopadhyay, Banibrata1 (AUTHOR)
Publikováno v:
Astronomy Reports. 2023 Suppl 2, Vol. 67, pS179-S188. 10p.