![]() |
|
1 Attachment(s)
|
I like pink 3 times more than yellow.
|
1 Attachment(s)
|
What a coincidence, I have 3 children!!!
|
I like spankings, & the one on the right.
|
I'm not sure who "they" are, but they must call me BadNick for a reason, or three.
|
1 Attachment(s)
|
I think "silly" would look better if it had 3 "L" in the middle, or at least more a onomonopia'ish. sillly
|
That's sillly. Where'd I put the tweezers?
|
I could tweeze her 3 times.
|
1 Attachment(s)
|
1 Attachment(s)
|
let me give them a hand, or three
|
Do you have any left-overs?
|
I'll split it with you. Right down the middle. We each get 3 halves.
|
1 Attachment(s)
|
I remember eyeing those, distracted by the tongues.
|
To keep it relevant to this thread, I just used a ruler to measure my tongue and it is more than 3" long before I start gagging on the ruler.
|
1 Attachment(s)
|
relevant rulers
never gag all their minions, just those who make sense. |
gag me wit a poon
|
...how far in did you say the ruler went?
|
I'm already getting sorry I said.
|
1 Attachment(s)
|
is there no end to silly girls? I hope not.
|
i miss sillygirl........
|
so do I. she was 3-D.
|
I like them most when they have dimensions. 3-D is good ...perhaps we can consider a 4 or 5 thread some day.
|
Where becomes a point.
|
point? Out, damn'd spot!!!
Extragalactic Radio Sources and the WMAP Cold Spot Authors: Lawrence Rudnick, Shea Brown, Liliya R. Williams (Submitted on 6 Apr 2007 (v1), last revised 3 Aug 2007 (this version, v2)) Abstract: We detect a dip of 20-45% in the surface brightness and number counts of NVSS sources smoothed to a few degrees at the location of the WMAP cold spot. The dip has structure on scales of approximately 1-10 degrees. Together with independent all-sky wavelet analyses, our results suggest that the dip in extragalactic brightness and number counts and the WMAP cold spot are physically related, i.e., that the coincidence is neither a statistical anomaly nor a WMAP foreground correction problem. If the cold spot does originate from structures at modest redshifts, as we suggest, then there is no remaining need for non-Gaussian processes at the last scattering surface of the CMB to explain the cold spot. The late integrated Sachs-Wolfe effect, already seen statistically for NVSS source counts, can now be seen to operate on a single region. To create the magnitude and angular size of the WMAP cold spot requires a ~140 Mpc radius completely empty void at z<=1 along this line of sight. This is far outside the current expectations of the concordance cosmology, and adds to the anomalies seen in the CMB. |
1 Attachment(s)
|
all 3 of their ages added together would be less than mine. Perfect!
|
1 Attachment(s)
|
|
random reflections
through mediums travelling are joys we can share |
|
1 Attachment(s)
|
brings new meaning to lipstick on a pig....
|
Tattooed pork tenderloins?
|
1 Attachment(s)
|
All times are GMT -8. The time now is 01:16 AM. |
|
Powered by vBulletin® Version 3.8.7
Copyright ©2000 - 2025, vBulletin Solutions, Inc.
Search Engine Optimization by vBSEO 3.6.0 PL2
© 2002-2012 Tilted Forum Project