... 36:02:09.6) (l II b II ) (185.12, +65.43) Spectral Type dM2 Distance 2.55 pc m V 7 m :49 B \Gamma V 1.51 [m=H 0.35 ROSAT/PSPC 0.18 cts s \Gamma1 EUVE/DS 0.02 cts s \Gamma1 EUVE Observation Mar 1995 [338.7 ks] Emission due to lines of different species ...
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Ссылки http://hea-www.harvard.edu/PINTofALE/papers/kgd_MM_head32_4217.ps.gz -- 256.6 Кб -- 03.11.2000 Похожие документы
... This work was supported by NASA Chandra award number G06-7073A. ChASeM33 Point Source Catalog We ran the CIAO tool wavdetect on data of each field in the bands S=0.35-1.1 keV, M=1.1-2.6keV, H=2.6-8.0 keV, and B=0.35-8.0 keV to perform source detection. ...
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Ссылки http://hea-www.harvard.edu/vlp_m33_public/sasaki_poster.pdf -- 1065.4 Кб -- 26.09.2007 Похожие документы
... an X-ray gas mass of 4300 M and an unabsorbed (0.35 2.5 keV) X-ray luminosity of ... m" (1.1-2.6keV) 40.0s 30.0s 20.0s 10.0s 30d47m00.0s 50.0s 40.0s 32.0s 1h34m30.0s 36 ...
... initial stellar mass function ( IMF ) (M ) ј AM ю2:35 (Salpeter 1955 ), where the ... Then R Msup Ni ј A Minf M ю2:35 dM , where Minf and Msup are, respectively, 0.7 M ...
... The focal plane FPC has an Aperture Plate, filled with twenty circular apertures, ranging from 3 Їm to 35mm in diameter, and fourteen slits (designed for grating and Ring Focus measurements), ranging between 5 and 500 Їm wide. ...