缓和紧张状况
发表于 2025-3-21 17:59:46
书目名称Disc Winds Matter影响因子(影响力)<br> http://impactfactor.cn/if/?ISSN=BK0280897<br><br> <br><br>书目名称Disc Winds Matter影响因子(影响力)学科排名<br> http://impactfactor.cn/ifr/?ISSN=BK0280897<br><br> <br><br>书目名称Disc Winds Matter网络公开度<br> http://impactfactor.cn/at/?ISSN=BK0280897<br><br> <br><br>书目名称Disc Winds Matter网络公开度学科排名<br> http://impactfactor.cn/atr/?ISSN=BK0280897<br><br> <br><br>书目名称Disc Winds Matter被引频次<br> http://impactfactor.cn/tc/?ISSN=BK0280897<br><br> <br><br>书目名称Disc Winds Matter被引频次学科排名<br> http://impactfactor.cn/tcr/?ISSN=BK0280897<br><br> <br><br>书目名称Disc Winds Matter年度引用<br> http://impactfactor.cn/ii/?ISSN=BK0280897<br><br> <br><br>书目名称Disc Winds Matter年度引用学科排名<br> http://impactfactor.cn/iir/?ISSN=BK0280897<br><br> <br><br>书目名称Disc Winds Matter读者反馈<br> http://impactfactor.cn/5y/?ISSN=BK0280897<br><br> <br><br>书目名称Disc Winds Matter读者反馈学科排名<br> http://impactfactor.cn/5yr/?ISSN=BK0280897<br><br> <br><br>
strain
发表于 2025-3-21 20:53:22
2190-5053 that supports a disc-wind based unification scenario for quasars. Lastly, the thesis also includes a theoretical investigation into the equivalent width distribution of the emission lines in quasars, which reveals a major challenge to all unification scenarios..978-3-319-86563-8978-3-319-59183-4Series ISSN 2190-5053 Series E-ISSN 2190-5061
精美食品
发表于 2025-3-22 00:38:46
James MatthewsNominated as an outstanding PhD thesis by the University of Southampton, Southampton, UK.Includes a broad introduction to accretion and outflow in astrophysical systems.Features a detailed description
nocturia
发表于 2025-3-22 06:49:12
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委屈
发表于 2025-3-22 09:45:18
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独行者
发表于 2025-3-22 13:12:39
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独行者
发表于 2025-3-22 17:05:01
Aphabetical Index of substances,Observational evidence for mass-loaded outflows or winds is widespread across the entire astrophysical mass range and most of the electromagnetic spectrum.
Musket
发表于 2025-3-22 21:24:23
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aggravate
发表于 2025-3-23 01:41:06
Space groups (194) P63/mmc - (190) P-62cHere, I present Monte Carlo radiative transfer simulations designed to assess the likely impact of accretion disc winds on the optical spectra of high-state CVs.
蚀刻
发表于 2025-3-23 07:22:16
Space groups (189) P-62m – (174) P-6In Chaps. . and ., I reviewed the observational evidence for accretion disc winds in quasars and luminous AGN, and showed how they may be responsible for more than just the broad absorption lines and P-Cygni profiles seen in quasar spectra.