u2

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Cosmic microwave background radiation, Leo, RA, DEC

http://www.google.dk/search?hl=da&q=Cosmic+microwave+background+radiation%2C+Leo%2C+RA%2C+DEC&btnG=S%C3%B8g&meta=

(4,38 MByte)

http://prl.aps.org/files/RevModPhys.79.1349.pdf

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[ site 10 of 31 ]

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> The current best observed dipole (3.358±0.017 mK) indicates

> that the solar system is moving at 368±2 km/sec relative to

> the observable universe in the direction galactic longitude

> l =263.86° and latitude b=48.25°

> with an uncertainty slightly smaller than 0.1° (Jarosik et al., 2006. )

> This is quite far from the galactic rotation direction (nominally 250 km/ s toward l=90° and b=0°).

(226 KByte)

http://huterer8.physics.lsa.umich.edu/~huterer/Papers/lowell.pdf

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[ site 1 of 4 ]

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> ... WMAP ... l = 263.85° ± 0.1°, b = 48.25° ± 0.04° in galactic coordinates

(4,328 MByte)

http://lambda.gsfc.nasa.gov/product/map/pub_papers/firstyear/basic/wmap_basic_results.pdf

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[ site 26 of 41 ]

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> 7.1. l = 1 dipole

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> COBE ...

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> ... 263.85 0.1, 48.25 0.04).