祈求
发表于 2025-3-21 16:37:33
书目名称Iron Line Diagnostics in X-ray Sources影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0475390<br><br> <br><br>书目名称Iron Line Diagnostics in X-ray Sources影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0475390<br><br> <br><br>书目名称Iron Line Diagnostics in X-ray Sources网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0475390<br><br> <br><br>书目名称Iron Line Diagnostics in X-ray Sources网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0475390<br><br> <br><br>书目名称Iron Line Diagnostics in X-ray Sources被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0475390<br><br> <br><br>书目名称Iron Line Diagnostics in X-ray Sources被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0475390<br><br> <br><br>书目名称Iron Line Diagnostics in X-ray Sources年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0475390<br><br> <br><br>书目名称Iron Line Diagnostics in X-ray Sources年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0475390<br><br> <br><br>书目名称Iron Line Diagnostics in X-ray Sources读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0475390<br><br> <br><br>书目名称Iron Line Diagnostics in X-ray Sources读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0475390<br><br> <br><br>
Palatial
发表于 2025-3-22 00:03:24
Thermal X-ray emission from centre-filled supernova remnants,evealed). Deprojection analyses of the X-ray images have been performed under simplfying assumptions and radial density distributions derived. These are inconsistent with a simple Sedov model, but are more similar to predictions of models involving evaporation of cold ISM clouds in the remnant centre.
Climate
发表于 2025-3-22 01:20:04
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食草
发表于 2025-3-22 04:53:04
Behaviour of the iron line in Cygnus X-1 during dips and persistent emission, dips. For one dip a broad emission line (FWHM ~ 2.6 keV) at 5.8 keV can be seen. This behaviour is discussed in terms of Comptonisation of the incident X-rays in relatively cold material, possibly associated with the stellar wind of the secondary.
Interregnum
发表于 2025-3-22 10:55:29
Conference proceedings 1991n studying the regions aroundblackholes and neutron stars. In this book the state of the artand themost recent theoretical and experimentalobservations are presented. Thebook will be a valuablesource for future satellite missions. It addressesbothresearchers and graduate students in astrophysics.
射手座
发表于 2025-3-22 12:58:13
0075-8450 stics ofhot plasmas in X-raysources. Their strength and purity allow importantconclusions to be drawn even with modest energy resolution.They should also help in studying the regions aroundblackholes and neutron stars. In this book the state of the artand themost recent theoretical and experimentalo
Dorsal-Kyphosis
发表于 2025-3-22 19:21:12
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伪造
发表于 2025-3-22 21:54:43
Iron L-shell line formation in diverse astrophysical environments,l processes that underlie the diagnostic potential of these features. We specifically consider corona) plasmas, X-ray photoionized nebulae, and the ionizing plasmas believed to be present in young supernova remnants.
歌唱队
发表于 2025-3-23 03:34:03
0075-8450 bservations are presented. Thebook will be a valuablesource for future satellite missions. It addressesbothresearchers and graduate students in astrophysics.978-3-662-13817-5978-3-540-47583-5Series ISSN 0075-8450 Series E-ISSN 1616-6361
Aggrandize
发表于 2025-3-23 06:07:52
Iron lines in X-ray spectra of high mass X-ray binaries, component of the spectrum the derived Fe column densities to explain the line intensity are consistent with the equivalent H column densities causing the photo-electric absorption of the low-absorption component.