... dark rings are not devoid of emission, and we estimate a grain emissivity index of 0 ... TB of all of the dark rings falls below Tm , consistent with the dark rings being ...
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Ссылки http://www.mrao.cam.ac.uk/~bn204/publications/2015/1503.02649v3.pdf -- 401.3 Кб -- 04.03.2016 Похожие документы
... The areas surrounded by the dark border will be mapped in the wide, shallow sur vey ... and isolated star formation regions selected from dark cloud catalogs (e.g., Lynds ... 10.--Extinction map of the Pipe Nebula. Details as in Fig. 3. Fig. ...
... Radio: Distorted shell, brighter to the E, with pulsar and associated nebula. ... X-ray: Centrally concentrated, thermal spectrum, plus pulsar nebula. ... VLA at 1.5 and 8.4 GHz (8 .9 в 7 .8) of pulsar nebula. Frail et al. ...
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Ссылки http://www.mrao.cam.ac.uk/projects/surveys/snrs-2001/table-IV-l.pdf -- 231.3 Кб -- 07.01.2002 Похожие документы
... Radio: Distorted shell, brighter to the E, with pulsar and associated nebula. ... X-ray: Centrally concentrated, thermal spectrum, plus pulsar nebula. ... VLA at 1.5 and 8.4 GHz (8 .9 в 7 .8) of pulsar nebula. Frail et al. ...
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Ссылки http://www.mrao.cam.ac.uk/projects/surveys/snrs-2001/table-IV.pdf -- 229.8 Кб -- 07.01.2002 Похожие документы
... Radio: Distorted shell, brighter to the E, with pulsar and associated nebula. ... X-ray: Centrally concentrated, thermal spectrum, plus pulsar wind nebula. ... VLA at 1.5 and 8.4 GHz (8 .9 в 7 .8) of pulsar nebula. Frail et al. ...
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Ссылки http://www.mrao.cam.ac.uk/projects/surveys/snrs-2004/table-IV.pdf -- 290.8 Кб -- 10.01.2005 Похожие документы
... Radio: Distorted shell, brighter to the E, with pulsar and associated nebula. ... X-ray: Centrally concentrated, thermal spectrum, plus pulsar wind nebula. ... VLA at 1.5 and 8.4 GHz (8 .9 в 7 .8) of pulsar nebula. Frail et al. ...
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Ссылки http://www.mrao.cam.ac.uk/projects/surveys/snrs-2004/table-IV-l.pdf -- 295.6 Кб -- 10.01.2005 Похожие документы
... Radio: Distorted shell, brighter to the E, with pulsar and associated nebula. ... Xray: Centrally concentrated, thermal spectrum, plus pulsar wind nebula. ... VLA at 1.5 and 8.4 GHz (8 ## .9в7 ## .8) of pulsar nebula. Frail et al. ...
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Ссылки http://www.mrao.cam.ac.uk/projects/surveys/snrs-2004/table-IV.ps -- 489.0 Кб -- 10.01.2005 Похожие документы
... Radio: Distorted shell, brighter to the E, with pulsar and associated nebula. ... Xray: Centrally concentrated, thermal spectrum, plus pulsar wind nebula. ... VLA at 1.5 and 8.4 GHz (8 ## .9в7 ## .8) of pulsar nebula. Frail et al. ...
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Ссылки http://www.mrao.cam.ac.uk/projects/surveys/snrs-2004/table-IV-l.ps -- 489.7 Кб -- 10.01.2005 Похожие документы
... Radio: Distorted shell, brighter to the E, with pulsar and associated nebula. ... Xray: Centrally concentrated, thermal spectrum, plus pulsar nebula. ... VLA at 1.5 and 8.4 GHz (8 00 :9 7 00 :8) of pulsar nebula. Frail et al. ...
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Ссылки http://www.mrao.cam.ac.uk/projects/surveys/snrs-2001/table-IV-l.ps -- 437.0 Кб -- 07.01.2002 Похожие документы
... Radio: Distorted shell, brighter to the E, with pulsar and associated nebula. ... Xray: Centrally concentrated, thermal spectrum, plus pulsar nebula. ... VLA at 1.5 and 8.4 GHz (8 00 :9 7 00 :8) of pulsar nebula. Frail et al. ...
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Ссылки http://www.mrao.cam.ac.uk/projects/surveys/snrs-2001/table-IV.ps -- 436.8 Кб -- 07.01.2002 Похожие документы