... ROSAT // Лутовинов А.А., Вихлинин А.А., Чуразов Е.М., Ревнивцев М.Г., Сюняев Р.А. Представлены результаты исследования скопления Галактик в созвездии Волосы Вероники (Coma cluster) в широком диапазоне энергий по данным обсерваторий ИНТЕГРАЛ, RXTE и ROSAT ...
... J114358.1-610736 had been proposed ([3]), we first took a spectrum of the only star within the error circle of the ROSAT source (about 1" from the nominal position of the ROSAT source), namely USNO-B1.0 0288-0337417 (RA: 11h 43m 58.5s , Decl: -61 07' 37 ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/G52_Torrejon01-26Apr07_13:48:22.pdf -- 108.1 Кб -- 26.04.2007 Похожие документы
... 4.1 X-RAY: The ROSAT Catalogues The primary catalogues used are those of the ROSAT Bright [8] and Faint [9] Source Catalogues, containing over 18000 and 100,000 sources respectively. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/E36_Stephen01-07May07_17:57:56.pdf -- 317.3 Кб -- 07.05.2007 Похожие документы
... panel) and 1RXH J190140.1+012630 (obtained by ROSAT/HRI, 0.1-2.4 keV, right panel ... During the pointed ROSAT/HRI observation performed on October 3, 1994, the source ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/E30_Karasev01-27Mar07_15:40:32.pdf -- 209.0 Кб -- 18.06.2007 Похожие документы
... However, this work is based on the ROSAT All-Sky Survey cluster sample, and so it ... sample, derived from a sensitive survey based on the ROSAT pointed observations [1 ...
... in 2004 Chandra followup underway check out poster A1 Data for distant clusters A1651, z = 0.085, ROSAT CL 1221+4918, z = 0.70, Chandra -1 s-1 keV -1 10 -2 -- comparable to ROSAT and ASCA uncertainties for low-z clusters f , cnt 10 -4 T/T 10%, M g /M g 20 ...