Titlebook: Non-Solar X- and Gamma-Ray Astronomy; L. Gratton Book 1970 International Astronomical Union 1970 astronomy.instruments.neutron star.observ

异国

书目名称Non-Solar X- and Gamma-Ray Astronomy影响因子(影响力)




书目名称Non-Solar X- and Gamma-Ray Astronomy影响因子(影响力)学科排名




书目名称Non-Solar X- and Gamma-Ray Astronomy网络公开度




书目名称Non-Solar X- and Gamma-Ray Astronomy网络公开度学科排名




书目名称Non-Solar X- and Gamma-Ray Astronomy被引频次




书目名称Non-Solar X- and Gamma-Ray Astronomy被引频次学科排名




书目名称Non-Solar X- and Gamma-Ray Astronomy年度引用




书目名称Non-Solar X- and Gamma-Ray Astronomy年度引用学科排名




书目名称Non-Solar X- and Gamma-Ray Astronomy读者反馈




书目名称Non-Solar X- and Gamma-Ray Astronomy读者反馈学科排名

使激动

U. R. Rao,E. V. Chitnis,A. S. Prakasarao,U. B. Jayanthi

悲痛

assent

P. C. Agrawal,S. Biswas,G. S. Gokhale,V. S. Iyengar,P. K. Kunte,R. K. Manchanda,B. V. Sreekantan

groggy

S. Hayakawa,T. Kato,F. Makino,H. Ogawa,Y. Tanaka,K. Yamashita,M. Matsuoka,S. Miyamoto,M. Oda,Y. Ogaw

Lumbar-Spine

M. Matsuoka,S. Miyamoto,J. Nishimura,M. Oda,Y. Ogawara,M. Wada

collateral

REP

熟练

Sudden Changes in the Intensity of High Energy X-rays from Sco X-1, an angle of 32° with respect to the zenith. A pair of crossed flux gate magnetometers provided information every 8.2 sec on the azimuth of the telescope. The pulse heights from the X-ray detector were sorted into several channels extending from 10 to 120 keV. An Am. source came into the field of vi

FADE

Intensities and Spectra of Several Galactic X-ray Sources,