... CTI/Gain (KD, MK by 15.01.2007) --> observation needed --> value from CC is 0.43,, not confirmed by Eta Carinae (but doubtful obs) consistent with 1e0102 --> archive CAS should be check to available with different temperatures TASK 036: REPORT ON MOS ...
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Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200704/Kirsch4.pdf -- 1052.9 Кб -- 13.05.2014 Похожие документы
... HD 148937 is surrounded by the circumstellar nebula NGC 616465, expanding with a pro jected velocity of about 30 km/s, and it is assumed that this nebula has been ejected during an LBVlike event (Leitherer & Chavarria, 1987). ...
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Ссылки http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p157.pdf -- 115.5 Кб -- 11.08.2011
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Ссылки http://mavr.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p157.pdf -- 115.5 Кб -- 11.08.2011 Похожие документы
... OB stars at the core of the Orion Nebula Cluster, and it represents a perfect ... Introduction The Orion Nebula (M42) is one of the closest (d 400-450 pc) and most ... Stauffer 1994; Hillenbrand 1997), which is known as the Orion Nebula Cluster (ONC ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2009/2009A&A...497..195K.pdf -- 1563.5 Кб -- 18.05.2009
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Ссылки http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2009/2009A&A...497..195K.pdf -- 1563.5 Кб -- 24.02.2010
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Ссылки http://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2009/2009A&A...497..195K.pdf -- 1563.5 Кб -- 24.02.2010 Похожие документы
... shaped HII region Gum 31 in the Carina region, with the aim of determining the main ... J1819-1458; observations have revealed absorption features and a bright X-ray nebula ... Velocity Structure in the Orion Nebula. II. ...