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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 showcase mean radius of 0.43 ± 0.3R ⊙, a gravity, log g = 5.0 ± 0.3, and that it nearly fills its Roche lobe

First high-resolution Chandra LETGS spectrum of the transient supersoft X-ray source RX J0513.9-6951

The double-degenerate nucleus of the planetary nebula TS01: A close binary evolution showcase mean radius of 0.43 ± 0.3R ⊙, a gravity, log g = 5.0 ± 0.3, and that it nearly fills its Roche lobe

First high-resolution Chandra LETGS spectrum of the transient supersoft X-ray source RX J0513.9-6951

Fine structure of density ducts formed by active radiofrequency action on laboratory and space plasmas

Fine structure of density ducts formed by active radiofrequency action on laboratory and space plasmas

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