Artigo Revisado por pares

Highlights from the KVANT mission

1990; Elsevier BV; Volume: 10; Issue: 2 Linguagem: Inglês

10.1016/0273-1177(90)90116-h

ISSN

1879-1948

Autores

R. Sunyaev, E. Churazov, V. V. Efremov, M. Gilfanov, С. А. Гребенев, A. S. Kaniovsky, D. Stepanov, S. Yunin, A. V. Kuznetsov, A. S. Melioransky, N. Yamburenko, S.S. Kiselev, I. Lapshov, N. Yu. Pappe, M. N. Boyarsky, В. М. Лозников, AF Prudkoglyad, O. Terekhov, C. Reppin, W. Pietsch, J. Englhauser, J. Trümper, W. Voges, E. Kendziorra, M. Bezler, R. Staubert, A. C. Brinkman, J. Heise, J. J. M. in ’t Zand, R. Jäger, G. K. Skinner, O. Al-Emam, T. G. Patterson, A. P. Willmore, A. J. Smith, A. N. Parmar,

Tópico(s)

Astro and Planetary Science

Resumo

The International X-ray observatory RÖNTGEN, aboard the KVANT module docked to the MIR space station, performed already more than 1000 sessions of observations of HER X-1, CYG X-1, CYG X-3, NGC 4151, CEN A, 3C 273, ASM 2000+25 and some other sources. The main target was SN1987a and the Large Magellanic Cloud field. Some results of observations (hard X-ray spectra, X-ray imaging and timing) are presented.

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