polysomnography
发表于 2025-3-21 17:49:36
书目名称Short-Period Binary Stars: Observations, Analyses, and Results影响因子(影响力)<br> http://impactfactor.cn/if/?ISSN=BK0866741<br><br> <br><br>书目名称Short-Period Binary Stars: Observations, Analyses, and Results影响因子(影响力)学科排名<br> http://impactfactor.cn/ifr/?ISSN=BK0866741<br><br> <br><br>书目名称Short-Period Binary Stars: Observations, Analyses, and Results网络公开度<br> http://impactfactor.cn/at/?ISSN=BK0866741<br><br> <br><br>书目名称Short-Period Binary Stars: Observations, Analyses, and Results网络公开度学科排名<br> http://impactfactor.cn/atr/?ISSN=BK0866741<br><br> <br><br>书目名称Short-Period Binary Stars: Observations, Analyses, and Results被引频次<br> http://impactfactor.cn/tc/?ISSN=BK0866741<br><br> <br><br>书目名称Short-Period Binary Stars: Observations, Analyses, and Results被引频次学科排名<br> http://impactfactor.cn/tcr/?ISSN=BK0866741<br><br> <br><br>书目名称Short-Period Binary Stars: Observations, Analyses, and Results年度引用<br> http://impactfactor.cn/ii/?ISSN=BK0866741<br><br> <br><br>书目名称Short-Period Binary Stars: Observations, Analyses, and Results年度引用学科排名<br> http://impactfactor.cn/iir/?ISSN=BK0866741<br><br> <br><br>书目名称Short-Period Binary Stars: Observations, Analyses, and Results读者反馈<br> http://impactfactor.cn/5y/?ISSN=BK0866741<br><br> <br><br>书目名称Short-Period Binary Stars: Observations, Analyses, and Results读者反馈学科排名<br> http://impactfactor.cn/5yr/?ISSN=BK0866741<br><br> <br><br>
透明
发表于 2025-3-21 22:22:56
Modeling the Hot Components in Cataclysmic Variables: Info on the White Dwarf and Hot Disk from GALEis visible and may be directly studied. Recent results from studies of this type have determined that pulsating white dwarfs in accreting systems exist in a different instability strip than single pulsators and that highly magnetic white dwarfs still have hot spots even when the mass transfer stream has ended.
clarify
发表于 2025-3-22 01:59:53
http://reply.papertrans.cn/87/8668/866741/866741_3.png
因无茶而冷淡
发表于 2025-3-22 05:35:34
0067-0057these objects are analyzed.Among the specific objects repor.Short-period binaries run the gamut from widely separated stars to black-hole pairs; in between are systems that include neutron stars and white dwarfs, and partially evolved systems such as tidally distorted and over-contact systems. Thes
Addictive
发表于 2025-3-22 08:46:31
http://reply.papertrans.cn/87/8668/866741/866741_5.png
音乐戏剧
发表于 2025-3-22 15:05:13
http://reply.papertrans.cn/87/8668/866741/866741_6.png
种属关系
发表于 2025-3-22 18:44:00
Gravitational Lensing in Compact Binary Systemsise due to time delays and magnification factors occurring as a result of gravitational lensing by other compact objects. The results are applied to the double pulsar PSR J0737-3039 to determine whether or not anomalous enhancements observed during the eclipse of pulsar A by pulsar B have the signat
Obstruction
发表于 2025-3-22 22:57:24
Accreting Neutron Stars in Low-Mass X-Ray Binary Systemsnct types of high-frequency X-ray oscillations. These oscillations are powered by release of the binding energy of matter falling into the strong gravitational field of the star or by the sudden nuclear burning of matter that has accumulated in the outermost layers of the star. The frequencies of th
SOW
发表于 2025-3-23 02:47:16
http://reply.papertrans.cn/87/8668/866741/866741_9.png
食道
发表于 2025-3-23 05:33:51
http://reply.papertrans.cn/87/8668/866741/866741_10.png