... the degree to which M SN пt constrains the 60 1.0 relative probability 0.8 0.6 0.4 ... 1.0 relative probability 0.8 0.6 0.4 0.2 0.0 -20.5 Fit0.25 Fit0.50 m=0.25 mag m=0.50 ...
... limit at near-infrared wavelengths of the Gemini South 8m telescope in Chile ... With Japanese collaborators, using the 8-m Subaru telescope, Freeman and Arnaboldi ... Dr M de Kool The Catholic University of America, Washington, March 8-10. ...
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Ссылки http://www.mso.anu.edu.au/annualReport/2001/annrep_2001.pdf -- 398.8 Кб -- 15.10.2004 Похожие документы
... 19 Table 7: Hi Rotation Curve for NGC 24 Radius (arcsec) 40 80 120 160 Vrot ( k m s -1 ) 56.6 82.5 91.8 99.2 Error ( k m s -1 ) 6.4 2.7 0.8 0.8 Radius (arcsec) 200 240 280 320 Vrot ( k m s -1 ) 103.6 106.2 109.4 109.7 Error ( k m s -1 ) 2.2 1.8 3.5 2.0 ...
... If we exclude the galaxies with the worst пts the median M/L rises to 2.7 ^ 0.8. ... His models have an M/L of 2.4 at an age of 6 Gyr and an M/L of 2.7 at 8 Gyr. ...
... 0260 email: brian@mso.anu.edu.au Academic Qualifications: 1 1 1 1 9 9 9 9 9 9 88 3 2 9 9 : : : : Ph.D. in Astronomy, Harvard University A.M. in Astronomy, Harvard University B.S. in Physics, University of Arizona B.S. in Astronomy, University of Arizona ...
... Telescope Project, which is constructing two 8m telescopes in Hawaii and Chile ... Australian astronomers with their only assured access to 8m class telescopes ... Kool, M, Arav, N, Becker R. 4th Annual Stromlo AGN Workshop, Canberra, 8-10 December ...
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Ссылки http://www.mso.anu.edu.au/annualReport/1999/annualrep1999.pdf -- 1204.9 Кб -- 15.10.2004 Похожие документы
... k Bk dt c @ m @ xi 5 Energy density, Poynting flux and Maxwell stress tensor EM S i = = = = EM i B ij MM E ij = E2 + B2 = Electromagnetic energy density 8 c ij k Ej Bk = Poynting flux 4 Si = Electromagnetic momentum density 2 c 1 12 Bi Bj B ij = Magnetic ...