... Now, striking new evidence discovered in M31 and NGC 3379 suggests that the metal-poor outermost halo can be isolated at very large radii, R > 12Reff. ...
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... already taken (Minchin 1999), so I settled on naming it after Marcel Duchamp, another cubist, but also one of the first artists to work with "found ob jects". 8 http://astronomy.swin.edu.au/s2plot/ REFERENCES 31 References M.R. Calabretta and E.W. Greisen ...
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... Comparison between Centaurus A and FR-I type RG 3C 31 Centaurus A Mdust ~ 106 M sun ,T dust = 30-40 K (Leeuw & Eckart 2002) R(2 ... 1997) M(H2) ~ 1x109Msun, Mgas/Mdyn=0.03 3C 31 (D=70Mpc) Mdust = 107 Msun, T dust = 24 K (Muller et al. ...
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Ссылки http://www.atnf.csiro.au/research/cena/documents/presentations/okuda.pdf -- 1509.2 Кб -- 16.07.2009 Похожие документы
... Duc, Jonathan Braine and Elias Brinks, eds. On the nature of dwarf galaxies in the interacting group HCG 31 ґ Angel R. Lґpez-Sґnchez & Cґsar Esteban o a e Instituto de Astrofґ ica de Canarias, E38200, Tenerife, Spain is Mґnica Rodrґ uez o ig INAOE, Apdo ...
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Ссылки http://www.atnf.csiro.au/people/Angel.Lopez-Sanchez/proceedings/sydney2003.pdf -- 74.8 Кб -- 03.02.2008 Похожие документы
... already taken (Minchin 1999), so I settled on naming it after Marcel Duchamp, another cubist, but also one of the first artists to work with "found ob jects". 8 http://astronomy.swin.edu.au/s2plot/ REFERENCES 31 References M.R. Calabretta and E.W. Greisen ...
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... 16 Figure 9 This spectr um obtained with a single 31-m baseline shows HCO+ absorption seen against the nucleus of the galaxy ... first obser vation as an interferometer working in the 3-mm band with a single 31-m baseline, between antennas 3 and 4 ...
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Ссылки http://www.atnf.csiro.au/the_atnf/annual_reports/2000/2000_AnnualReport.pdf -- 1644.7 Кб -- 29.11.2011 Похожие документы