带来
发表于 2025-3-28 17:27:55
Two new faint common proper motion pairs,warf and an m.=19.8 DC9 white dwarf separated by 23″. ES0440-55a/SSb has an m.=20.2 red dwarf (ST=M5.1) component and a DZ7 white dwarf with m.=19.3, their angular separation being 5.4". The proper 0447 17 motion of the pairs is μ=0.38±0.03″/year and μ=0.22±0.04″/year respectively.
落叶剂
发表于 2025-3-28 18:57:18
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ANNUL
发表于 2025-3-29 00:25:35
Conference proceedings 1989 current fields of research in this area are covered including the evolution of white dwarfs, links to progenitors, luminosity functions of white dwarfs, evolution of white dwarfs in binaries, spectroscopy and atmospheric abundances, diffusion, accretion and convective mixing, the mass-radius relati
晚来的提名
发表于 2025-3-29 06:49:44
0075-8450 8. All the current fields of research in this area are covered including the evolution of white dwarfs, links to progenitors, luminosity functions of white dwarfs, evolution of white dwarfs in binaries, spectroscopy and atmospheric abundances, diffusion, accretion and convective mixing, the mass-rad
容易做
发表于 2025-3-29 08:55:47
0075-8450of single white dwarfs. All the articles are by internationally known authorities and contain the most up-to-date information available at the time of writing.978-3-662-13745-1978-3-540-46136-4Series ISSN 0075-8450 Series E-ISSN 1616-6361
摊位
发表于 2025-3-29 13:33:59
An unsuccessful search for white dwarf companions to nearby main sequence stars, or M) main-sequence secondary, be visible in IUE images as a hot companion to the main sequence star. We systematically examined 318 IUE images of 280 different G, K, and M stars which had been observed for other purposes.No previously undiscovered white dwarf stars were found.
relieve
发表于 2025-3-29 17:40:16
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灌输
发表于 2025-3-29 23:44:38
The effects of time dependant convection on white dwarf radial pulsations, analysis stabilizes most of the modes in both the DA and DB radial instability strips. We also find that the blue edge of the DA radial instability strip, assuming frozen in convection, is between 12,000K and 13,000K. The blue edge for the DB radial instability strip (frozen in convection) is between 32,000K and 33,000K.
不愿
发表于 2025-3-30 02:02:07
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情爱
发表于 2025-3-30 04:54:04
Load-balancing procedure for distributed short-range molecular dynamics,.First, simulation of the cluster load has been used for tests of several load-balancing procedures. Then the chesen procedure has been applied in the MD algorithm executed on heterogeneous clusters of workstations during standard load.