... We also In all cases a stable circumbinary co-rotating envelope was formed after a few binary orbits. ... the envelope mass was replaced once per orbit giving 5.5 10-10 solar mass for its mass (assuming mass loss rate 10-6 solar mass ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/F39_Hjalmarsdotter02-17Apr07_14:19:21_bandw.pdf -- 212.8 Кб -- 17.04.2007 Похожие документы
... We also In all cases a stable circumbinary co-rotating envelope was formed after a few binary orbits. ... the envelope mass was replaced once per orbit giving 5.5 10-10 solar mass for its mass (assuming mass loss rate 10-6 solar mass ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/F39_Hjalmarsdotter02-17Apr07_14:19:21_color.pdf -- 192.4 Кб -- 17.04.2007 Похожие документы
... Paul Scherrer Institut,CH-5232 Villigen PSI, Switzerland, E-mail:wojtek.hajdas@psi.ch ABSTRACT The Reuven Ramaty High Energy Solar Spectroscopic Explorer (RHESSI) satellite [1] with its 9 large Ge detectors may be used as a rotating gamma ray polarimeter ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/I33_Hajdas02-09May07_09:01:42.pdf -- 188.7 Кб -- 09.05.2007 Похожие документы
... and VENERA-10: cloud layer, upper atmosphere and interaction with the solar wind ... Current sheet characteristics and thermal trigger of solar flares . ... Synthesis of circular apertures with rotating fixed base length two-element ...
... 24], the maximum particle energy, E max , observed in various particleacceleration cites, including the rotating neutron stars (NSs), as well as aurora sub-storms, solar flares, blazar jets, shell-like and Crab-like supernova remnants) generally scales as ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/H30_Terada01-07Feb07_06:25:26.pdf -- 537.5 Кб -- 07.02.2007 Похожие документы
... Usov 94 Thompson et al 94-06 92 crust · Slowly rotating, with X-ray emission powered by magnetic energy · Some magnetars also ... Resonant absorption in solar corona (Ionson 78, Hollweg 87, Steinolfson 85, etc.. ...
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Ссылки http://hea.iki.rssi.ru/conf/hea2010/Presentations/21/Levin.pdf -- 2594.3 Кб -- 26.01.2011 Похожие документы
... used Vt = 15 km/s and the solar chemistry: H = 1.00, He = 0.089 by mass logN(H)=12.00, logN(He) = 10.95 by number of atoms logN for the remaining elements: 8.52, N 8.01, O 8.89, Ne 8.05, Mg 7.54, Si 7.51, Fe 7.63 ROTATION VELOCITY FOR 1ORI C1 · v sini ...
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Ссылки http://hea.iki.rssi.ru/conf/hea2010/Presentations/24/Balega.pdf -- 453.0 Кб -- 26.01.2011 Похожие документы
... E.g. typical rotation period for a particle in the close vicinity of the 108 solar masses black hole is of an order of 105 seconds - i.e. about one day. ...
... Generically, the star formation rate (SFR, expressed in solar masses per year, M y-1 ... density (M y-1 kpc-2) in the solar neighborhood, and possibl y its radial dependence ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/B07_Hartmann01-07May07_12:04:00.pdf -- 279.4 Кб -- 07.05.2007 Похожие документы
... magnetars, the ROSAT-discovered "Magnificent Seven" (M7), rotating radio transients (RRATs), and central compact ob jects in ... emitting INS presenting exactly the same characteristics as the M7 has been identified outside the solar vicinity to date ...