Titlebook: Iron Line Diagnostics in X-ray Sources; Proceedings of a Wor A. Treves,G. C. Perola,L. Stella Conference proceedings 1991 Springer-Verlag B

祈求

书目名称Iron Line Diagnostics in X-ray Sources影响因子(影响力)




书目名称Iron Line Diagnostics in X-ray Sources影响因子(影响力)学科排名




书目名称Iron Line Diagnostics in X-ray Sources网络公开度




书目名称Iron Line Diagnostics in X-ray Sources网络公开度学科排名




书目名称Iron Line Diagnostics in X-ray Sources被引频次




书目名称Iron Line Diagnostics in X-ray Sources被引频次学科排名




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书目名称Iron Line Diagnostics in X-ray Sources年度引用学科排名




书目名称Iron Line Diagnostics in X-ray Sources读者反馈




书目名称Iron Line Diagnostics in X-ray Sources读者反馈学科排名

Palatial

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

食草

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

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

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

伪造

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

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

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.