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    • 1. http://www.stecf.org/conferences/adass/adassVII/reprints/miebachm.ps.gz
    ... 00 2 ,0 E ­05 4 ,0 E ­05 19 .8 .97 22 :53 20 .8 .97 0 :05 20 .8 .97 1 :17 20 .8 .97 2 :29 20 .8 .97 3 :41 Magnetic Field [Tesla] Q598 QDV10MF0 10sec Magne tic F e ld 1 Q599 QDV10MF1 10sec M agne tic F e ld 2 Q600 QDV10MF2 10sec Magne tic F e ld 3 Figure 3 ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/miebachm.ps.gz -- 186.8 Кб -- 12.06.2006
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    2. Near IR Astronomy with the ESO VLT
    ... CONICA, SINFONI, VISIR, VLTI). Stars. Abundances, circumstellar shells, mass loss, magnetic fields (CRIRES, VISIR). Star formation. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node6.html -- 17.8 Кб -- 12.06.2006
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    3. A Parallel Procedure for the Analysis of Long-term Sequences of Light Curves
    ... Binary systems belonging to the RS CVn and BY Dra classes show huge cool spots on their photospheres which are regarded as manifestations of intense magnetic fields by analogy with sunspots (e.g., Tuominen et al. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/lanzaa.html -- 15.0 Кб -- 12.06.2006
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    4. http://www.stecf.org/conferences/adass/adassVII/reprints/lanzaa.pdf
    ... Introduction Binary systems belonging to the RS CVn and BY Dra classes show huge cool spots on their photospheres which are regarded as manifestations of intense magnetic fields by analogy with sunspots (e.g., Tuominen et al. ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/lanzaa.pdf -- 132.1 Кб -- 12.06.2006
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    5. http://www.stecf.org/coordination/esa_eso/galpops/report.pdf
    ... This is now explained by a threshold magnetic field of 104 ­105 Gauss, above which a ... most notably, convection) and the role of magnetic fields in stellar evolution ...
    [ Текст ]  Ссылки http://www.stecf.org/coordination/esa_eso/galpops/report.pdf -- 2038.4 Кб -- 04.09.2008
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    6. http://www.stecf.org/goods/esomess.ps
    ... fields selected are already amongst the most intensively studied areas of the deep `extragalactic' sky: HDF­N (around 12.6 hr ...
    [ Текст ]  Ссылки http://www.stecf.org/goods/esomess.ps -- 342.9 Кб -- 28.09.2001
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    7. http://www.stecf.org/coordination/esa_eso/extrasolar/report.pdf
    ... the orbits of planetary systems are randomly distributed in the Galaxy comes from the fact that stellar rotation axes are themselves randomly distributed (obtained by v sin i distributions, and independently confirmed by magnetic-field orientation studies ...
    [ Текст ]  Ссылки http://www.stecf.org/coordination/esa_eso/extrasolar/report.pdf -- 1083.5 Кб -- 04.09.2008
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    8. CONICA: The high resolution near-infrared camera for the ESO VLT
    ... 14 and 55 mas/pixel, corresponding to fields of view between 14x14 and 56x56 arcsec ... of about 110 mas/pixel which leads to a field of view of about 73 arcsec in diameter ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node7.html -- 16.6 Кб -- 12.06.2006
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    9. http://www.stecf.org/coordination/esa_eso/alma-herschel/report.pdf
    ... Field of View (') 1.75 by 3.5 1.75 by 3.5 1.75 by 3.5 Table 4: Some Characteristics of SPIRE Central Wavelength (m) 250 360 520 ...
    [ Текст ]  Ссылки http://www.stecf.org/coordination/esa_eso/alma-herschel/report.pdf -- 1000.5 Кб -- 04.09.2008
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    10. http://www.stecf.org/coordination/esa_eso/cosmology/report.pdf
    ... field is constant both spatially and temporally, the equation of state is then p ... widest-field spectroscopic facilities at the VLT are VIMOS, with a field of view of ...
    [ Текст ]  Ссылки http://www.stecf.org/coordination/esa_eso/cosmology/report.pdf -- 1894.6 Кб -- 04.09.2008
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