... Chandra Swift Integral GLAST 2006 NEXT .. ... 2020 2010 Energy band Integral XMM Chandra HXR Focus NEXT EXIST Con-X GLAST 0.1 X ... Evolution of SMBH over cosmic time Current Chandra/XMM surveys do not reach F peak ...
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Ссылки http://www.naic.edu/~astro/chicago2/talks/Harrison-HighEnergy-Radio_Connection.pdf -- 795.4 Кб -- 21.08.2006 Похожие документы
... Images of the SNR fields with the Chandra X-ray telescope have revealed unresolved sources with properties suggestive of rotation-powered pulsars with active magnetospheres that are powering these nebulae. ...
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Ссылки http://www.naic.edu/vscience/schedule/tpfiles/ArzoumaniantagP2777tp.pdf -- 50.9 Кб -- 19.09.2012 Похожие документы
... the Young Neutron Star in IC443 ABSTRACT: We request 6 hours of telescope time to search for the radio counterpart to the X-ray-bright neutron star CXOU J061705.3+222127 recently discovered with the Chandra observatory in the supernova remnant (SNR) IC443 ...
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Ссылки http://www.naic.edu/vscience/schedule/tpfiles/CamilotagP1560tp.ps -- 92.7 Кб -- 19.04.2004 Похожие документы
... Counterpart to the Neutron Star in SNR G54.1+0.3 ABSTRACT: We request 3 hours of telescope time to search for the radio counterpart to the X-ray-bright neutron star recently discovered with the Chandra observatory in the supernova remnant (SNR) G54.1+0.3 ...
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Ссылки http://www.naic.edu/vscience/schedule/tpfiles/CamilotagP1592tp.ps -- 93.5 Кб -- 19.04.2004 Похожие документы
... Counterpart to the Neutron Star in SNR G54.1+0.3 ABSTRACT: We request 3 hours of telescope time to search for the radio counterpart to the X-ray-bright neutron star recently discovered with the Chandra observatory in the supernova remnant (SNR) G54.1+0.3 ...
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Ссылки http://www.naic.edu/vscience/schedule/tpfiles/CamilotagP1599tp.ps -- 93.5 Кб -- 19.04.2004 Похожие документы
... from the Neutron Star in SNR G39.2-0.3 ABSTRACT: We request 2.5 hours of telescope time to search for the radio counterpart to the X-ray-bright neutron star (NS) recently discovered with the Chandra observatory in the supernova remnant (SNR) G39.2-0.3 ...
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Ссылки http://www.naic.edu/vscience/schedule/tpfiles/CamilotagP1637tp.ps -- 90.6 Кб -- 19.04.2004 Похожие документы
... We propose an alternative interpretation of the arcs in the nebular X-radiation observed by Pavlov et al (2000) Helfand et al (2001) with the Chandra Observatory, and interpreted by the latter as an equatorial wind. ...
... Sinha, H. S. S., R. N. Misra, H. Chandra, S. Raizada, N. Dutt, and G. D. Vyas, Multi-wavelength optical imaging of ionospheric ... Sridharan, R., H. Chandra, S. R. Das, R. Sekar, H. S. S. Sinha, D. Pallam Raju, R. Narayanan, S. Raizada, R. N. Misra, R ...
... A recent Chandra X-ray image obtained by us suggests a new interpretation of the available facts: a hard X-ray p oint source near the ap ex of the G70.7+1.2 b ow-sho ck structure is a young neutron star and, in all likeliho o d, an active radio pulsar. ...
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Ссылки http://www.naic.edu/vscience/schedule/tpfiles/ArzoumaniantagP2175tp.pdf -- 39.5 Кб -- 10.10.2005 Похожие документы