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		<identifier>8JMKD3MGP3W34T/48DSBTP</identifier>
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		<metadatalastupdate>2024:04.25.15.35.57 urlib.net/www/2021/06.04.03.40 simone {D 1969}</metadatalastupdate>
		<secondarykey>INPE--TDI/</secondarykey>
		<citationkey>Gonzalez-Alarcon:1969:AnXrDa</citationkey>
		<title>An analysis of x-ray data obtained from the source-SCO XR-1</title>
		<alternatetitle>x</alternatetitle>
		<course>CEA-SPG-INPE-BR</course>
		<year>1969</year>
		<date>1969-12</date>
		<thesistype>Dissertação (Mestrado em Ciência Espacial)</thesistype>
		<secondarytype>TDI</secondarytype>
		<numberofpages>49</numberofpages>
		<numberoffiles>2</numberoffiles>
		<size>4208 KiB</size>
		<author>Gonzalez-Alarcon, Walter Demétrio,</author>
		<committee>Bowyer, C. Stuart,</committee>
		<committee>Lampton, Michael,</committee>
		<e-mailaddress>walter.gonzalez@inpe.br</e-mailaddress>
		<university>Instituto Nacional de Pesquisas Espaciais (INPE)</university>
		<city>São José dos Campos</city>
		<transferableflag>1</transferableflag>
		<keywords>x.</keywords>
		<abstract>On June 22 of 1969 an Aerobe rocket was launched in Natal, Brazil, as a cooperatiVe program between the National Council of Space Activities of Brazil (CNAE) and the Space Sciences Laboratory of the University of California, Berkeley. The objective was to search for new galactic X-ray sources, to detect some of the known ones, and to study the interplanetary medium as an absorbing region for X-rays. In this work we present the analysis of the galactic source SCO XR-1 which has been detected during the experiment. We have found that the best model for SCO XR-1 is Thermal Bremsstrahlung from a Hot Plasma with a temperature corresponding to 9.8 Key and a column density of absorbing atoms of 1.8 x 10^21 atoms/cm^2 . The measured energy range goes from 0.1 Key to 10.0 Key.</abstract>
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		<language>en</language>
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		<url>http://mtc-m21d.sid.inpe.br/rep-/sid.inpe.br/mtc-m21d/2023/01.23.17.32</url>
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