Non-LTE models for neutron star atmospheres and supernova-fallback disks.35). Accordingly, this would result in NS mass and radius lower limits of M ≥ 1.63 Mȯ and
R ≥ 13.8 km. © 2006
Absorption features in the spectra of X-ray bursting neutron stars-radius ratio from the measured gravitational redshift. A radius of
R=9-12km for a plausible mass range of M= 1
Absorption features in the spectra of X-ray bursting neutron stars-radius ratio from the measured gravitational redshift. A radius of
R=9-12km for a plausible mass range of M= 1
Non-LTE models for neutron star atmospheres and supernova-fallback disks.35). Accordingly, this would result in NS mass and radius lower limits of M ≥ 1.63 Mȯ and
R ≥ 13.8 km. © 2006
The double-degenerate nucleus of the planetary nebula TS01: A close binary evolution showcaseTovmassian G.,
Yungelson L.,
Rauch T.,
Suleimanov V.,
Napiwotzki R.,
Stasińska G.,
Tomsick J.,
Wilms J.,
Morisset C.,
Pẽa M.,
Richer M. mean radius of 0.43 ± 0.3
R ⊙, a gravity, log g = 5.0 ± 0.3, and that it nearly fills its Roche lobe
The double-degenerate nucleus of the planetary nebula TS01: A close binary evolution showcaseTovmassian G.,
Yungelson L.,
Rauch T.,
Suleimanov V.,
Napiwotzki R.,
Stasińska G.,
Tomsick J.,
Wilms J.,
Morisset C.,
Pẽa M.,
Richer M. mean radius of 0.43 ± 0.3
R ⊙, a gravity, log g = 5.0 ± 0.3, and that it nearly fills its Roche lobe