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0320086

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DataCite Commons2025-03-14 更新2025-04-15 收录
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http://esdcdoi.esac.esa.int/doi/html/data/astronomy/integral/0320086.html
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We propose to use advantages of the INTEGRAL observatory -- excellentenergy resolution and high sensitivity of its telescopes in the hardX-rays -- to study primary eclipse light curve of SS433 andspectral changes during the eclipse in hard X-rays inprecessional phase 0.5. This should help to localize the HXRemission region and derive its structure comparing HXR behavior withthe well-known data in softer X-ray bands (Ginga RXTE) and giveimportant hints for determination of the binary system parameters. [truncated! Please see actual data for full text]
提供机构:
European Space Agency
创建时间:
2025-03-14
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