musicologist
发表于 2025-3-23 13:23:11
The Cool Components in Cataclysmic Variables: Recent Advances and New Puzzles containing a white dwarf primary and a low-mass secondary star. These old star systems interact via mass transfer from the Roche-Lobe filling secondary to the higher gravitational potential of the primary star. The white dwarf primary has a mass of 1.4 M.or less while the secondary object ranges fr
HAVOC
发表于 2025-3-23 15:13:29
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bourgeois
发表于 2025-3-23 20:00:12
Distance Estimation for Eclipsing X-ray Pulsarsitudes of the optical star via either of two standard magnitude calibrations that agree within 4 percent. Accordingly the corresponding distance disagreement (due to the calibrations only) is only 2 percent, which is negligible compared to several other error sources. The flux-distance scaling is no
Compassionate
发表于 2025-3-23 22:33:07
The Tools of the Trade and the Products they Produce: Modeling of Eclipsing Binary Observablesthat encompass the entire close-binary realm from unevolved binaries to black hole systems. The purpose of this portion of the volume is to report on results from systems less evolved than black–holes, neutron stars, and white dwarfs, and in doing this to emphasize both the current modeling techniqu
Apoptosis
发表于 2025-3-24 03:33:43
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minion
发表于 2025-3-24 08:01:24
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白杨
发表于 2025-3-24 14:02:14
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修剪过的树篱
发表于 2025-3-24 18:11:18
Searches for Gravitational Waves from Binary Neutron Stars: A Review binaries, including the theory, instrumentation and methods. No detections have been made to date. However, the best direct observational limits on coalescence rates have been set, and instrumentation and analysis methods continue to be refined toward the ultimate goal of defining the new field of gravitational wave astronomy.
TAIN
发表于 2025-3-24 20:01:59
978-90-481-7666-3Springer Science+Business Media B.V. 2008
Retrieval
发表于 2025-3-24 23:21:50
Short-Period Binary Stars: Observations, Analyses, and Results978-1-4020-6544-6Series ISSN 0067-0057 Series E-ISSN 2214-7985