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Results: 1-7 |
Results: 7
Is KPD 1930+2752 a good candidate type Ia supernova progenitor?
Authors: Ergma, E Fedorova, AV Yungelson, LR
Citation: E. Ergma et al., Is KPD 1930+2752 a good candidate type Ia supernova progenitor?, ASTRON ASTR, 376(1), 2001, pp. L9-L12
What can we learn from the surface chemical composition of the optical companions of Soft X-ray transients?
Authors: Ergma, E Sarna, MJ
Citation: E. Ergma et Mj. Sarna, What can we learn from the surface chemical composition of the optical companions of Soft X-ray transients?, ASTRON ASTR, 374(1), 2001, pp. 195-203
The helium white dwarf in two pulsars: too cool in PSR J0751+1807 and too hot in PSR J1012+5307?
Authors: Ergma, E Sarna, MJ Gerskevits-Antipova, J
Citation: E. Ergma et al., The helium white dwarf in two pulsars: too cool in PSR J0751+1807 and too hot in PSR J1012+5307?, M NOT R AST, 321(1), 2001, pp. 71-76
Cooling curves and initial models for low-mass white dwarfs (< 0.25 M-circle dot) with helium cores
Authors: Sarna, MJ Ergma, E Gerskevits-Antipova, J
Citation: Mj. Sarna et al., Cooling curves and initial models for low-mass white dwarfs (< 0.25 M-circle dot) with helium cores, M NOT R AST, 316(1), 2000, pp. 84-96
The eclipsing binary millisecond pulsar PSR B1744-24A - possible test for a magnetic braking mechanism
Authors: Ergma, E Sarna, MJ
Citation: E. Ergma et Mj. Sarna, The eclipsing binary millisecond pulsar PSR B1744-24A - possible test for a magnetic braking mechanism, ASTRON ASTR, 363(2), 2000, pp. 657-659
An evolutionary model for SAX J1808.4-3658
Authors: Ergma, E Antipova, J
Citation: E. Ergma et J. Antipova, An evolutionary model for SAX J1808.4-3658, ASTRON ASTR, 343(2), 1999, pp. L45-L48
From which stars black holes and neutron stars may form?
Authors: Ergma, E van den Heuvel, EPJ
Citation: E. Ergma et Epj. Van Den Heuvel, From which stars black holes and neutron stars may form?, PHYS SCR, T77, 1998, pp. 76-78
Risultati: 1-7 |