天鹅座X-1硬X射线的能量谱     

马宇蒨  李光华  张承模  钱跃民  肖谦益  陆柱国  吴枚  戴长江  李惕碚  顾逸东  张希元 《中国天文和天体物理学报》1989,(4)

1985年9月22日,我们用空间硬X射线望远镜HAPI-2,在我国的高空气球上,对天鹅座X-1进行了观测,望远镜几何面积为140cm~2,观测能区20—200keV,空间定向精度±0.2°。获得的硬X射线能谱陡,总辐射能流LX～1.0×1~(37)erg/sec,低于常规态。本文将介绍望远镜的性能和观测过程,能谱分析的结果,并对当时天鹅座X-1可能的“态”进行讨论。  相似文献   

Strontium isotope trends during diagenesis in ore-bearing carbonate basins     

H. Gorzawski  L. Fonboté  J. F. Sureau  J. Y. Calvez 《International Journal of Earth Sciences》1989,78(1):269-290

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Properties of the components of symbiotic stars deduced from model calculations     

L. É. Leédyarv 《Astrophysics》1989,31(2):598-606

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Book reviews     

Roy  B. K.  Stanley  William R.  Bronger  Dirk  Dlin  Norman  Kukliński  Antoni  Cori  Berardo  Babikir  A. A. A.  Kunkel  G.  César  N.  Martin  Kähler 《GeoJournal》1989,18(2):255-260

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Book review     

P. Kertész 《Rock Mechanics and Rock Engineering》1994,27(2):112-113

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Simultaneous spaced direction-finding measurements of medium-latitude VLF/ELF emissions     

M. Hayakawa  Y. Tanaka  A. Iwai  J. Ohtsu  L.R.O. Storey  C. Béghin  T.S. Jorgensen 《Planetary and Space Science》1981,29(5):505-520

Simultaneous spaced measurements of medium-latitude VLF/ELF emissions were carried out during the three northern winters from 1976 to 1979. The experiment was making use of two different kinds of direction-finding systems (a field-analysis method and a goniometer network) at two stations in Europe, namely Brorfelde in Denmark (L = 2.9) and Chambron-la-Foret in France (L = 1.9); this enabled us to locate the ionospheric exit regions of emissions over a wide range of L-values up to and beyond 4.0, the average plasmapause location. In order to study the time delay in the temporal evolution of VLF emissions or the longitudinal drift of the emissions, observations from the Moshiri Observatory in Japan, widely separated in longitude, are also used. The overall system of the VLF equipment installed at the three stations is described. Then we present the VLF/ELF data of good quality obtained during the final year's campaign (Nov. 1978–Feb. 1979). By making use of the direction-finding data, we were able to classify the observed emissions into several categories, and some early results for some of the emissions are presented.  相似文献   

A compact model for the planar rhomboidal 4-body problem     

Ernesto A. Lacomba  Ernesto Pérez-Chavela 《Celestial Mechanics and Dynamical Astronomy》1992,54(4):343-355

We obtain a compact model for the global study of the planar rhomboidal 4-body problem in a level of constant negative energy. This model is a variation of the non compact model obtained through a McGehee blow up transformation. but compactness permits to obtain results which are not clear in the other case.  相似文献   

Fourier analysis of the light curves of eclipsing variables with extended atmospheres     

Alvaro Giménez  José M. García-Pelayo 《Astrophysics and Space Science》1979,66(2):511-513

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White dwarfs: Connection with masses of the parent stars     

P. R. Amnuél'  O. Kh. Guseinov  Kh. I. Novruzova  Yu. S. Rustamov 《Astrophysics》1987,27(1):365-371

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Observations of the OH Radical in Comet C/1995 O1 (Hale-Bopp) with the Nançay Radio Telescope     

Colom  P.  Gérard  E.  Crovisier  J.  Bockelé-Morvan  D.  Biver  N.  Rauer  H. 《Earth, Moon, and Planets》1997,78(1-3):37-43

We present OH 18-cm observations of comet Hale-Bopp (C/1995 O1) at the Nançay radio telescope. On nucleus and offset position observations allowed us to obtain both OH production rates and quenching radii. The maximum OH production rate was reached around perihelion, at about10³¹ s^-1.  相似文献