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

異國

書目名稱Non-Solar X- and Gamma-Ray Astronomy影響因子(影響力)




書目名稱Non-Solar X- and Gamma-Ray Astronomy影響因子(影響力)學科排名




書目名稱Non-Solar X- and Gamma-Ray Astronomy網(wǎng)絡公開度




書目名稱Non-Solar X- and Gamma-Ray Astronomy網(wǎng)絡公開度學科排名




書目名稱Non-Solar X- and Gamma-Ray Astronomy被引頻次




書目名稱Non-Solar X- and Gamma-Ray Astronomy被引頻次學科排名




書目名稱Non-Solar X- and Gamma-Ray Astronomy年度引用




書目名稱Non-Solar X- and Gamma-Ray Astronomy年度引用學科排名




書目名稱Non-Solar X- and Gamma-Ray Astronomy讀者反饋




書目名稱Non-Solar X- and Gamma-Ray Astronomy讀者反饋學科排名

使激動

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

熟練

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,