Fratley

I consider the PS1 a classic console now, and there are plenty of smash hits that were exclusive to it. What was your favourite? Spyro the Dragon. Beat that. Can you? No. [spoiler]inb4 PS1 sucks, N64 wins. No, they both win.[/spoiler] :wub:

I left for 3 months, came back and everyone's still a prick. Nothing changes.

8's my favourite, 9's the best.

If you're allowed to shoot ANYONE for forcing their way into your property with mal-intent, then yeah you should be allowed to do it to the police as well. Good police officers won't barge into a residence without a warrant, which is already illegal, so what's the problem?

Found you a member. He's quite photogenic and wants to be your poster boy. [spoiler][/spoiler]

Don't have a steady job any more. But I occasionally make some money doing some session work with the drum kit. Recordings and performance productions and the like. I usually help out with university student projects. Would get something like £50 for an hour or two on the day. Demand for such things is understandably sparse though, so I hardly make a living of it.

[quote name='SgtAsh' timestamp='1367593885' post='318586'] Wut? [/quote] Damn yanks.

[quote name='Kelarr' timestamp='1365533301' post='275568'] That's the point. [/quote] AAAAAAAAAAAAAH

0/10 everything for being a defensive bastard. I GAVE YOU GOOD SCORES, DAMMIT

8/10 Avatar. -2 because it creeps me the fuck out. 9/10 Signature. I do like those hand drawn ones. -1 because I can't read the really light grey text without tipping my screen up.

[quote name='Squall' timestamp='1365525661' post='275369'] ;_; Fine fine I changed it ;__; I gotta admit that this Avatar looks a 1000x better than the previous one ;3 Also my rating for Aziz: Avatar- 4/10, not really my type of Avatar. Sig- 3/10 because I am not that fond of Pokemon. Three points were given because Sonic put an effort into making that sig. [/quote] My new rating for your Avatar is 10/10

[img]http://i1326.photobucket.com/albums/u644/Fratley/ok_zps43689ebb.png[/img]

[quote name='Squall' timestamp='1365520438' post='275235'] The ribbon looks really good on you ;3 Edit: Ribbons honestly won't look good on many grills, it fits you for some reason though. And also my rating: Avatar: 10/10 Sig: 2/10 coz I am not fond of Pokemon. [/quote] My rating: 0/10 for Avatar. I demand that you use the original Squall portrait from FF8 and not that gay Dissidia bullshit! 8/10 for Sig. You win 8 points for having snapshots from FF8 as photographs in the background. That's... [size=1]that's kinda cool[/size].

[quote name='CipherWeston' timestamp='1365474800' post='274395'] [img]http://i.imgur.com/Xqrpda8.png[/img] Yes. [/quote] Lame.

[quote name='CipherWeston' timestamp='1365474613' post='274389'] If the picture would've worked, I wouldn't have had to click on the picture to see it. That's all I'm saying. The picture brought me to Funnyjunk, and a total of zero people on these forums like funnyjunk. [/quote] You had to click on it to see it?

[quote name='CipherWeston' timestamp='1365474116' post='274356'] I'm not implying anything. I'm saying the picture is from Funnyjunk, and funnyjunk is shit. [/quote] Wrong. The picture is from Google. Get your shit together, bitch! [img]http://ronanwills.files.wordpress.com/2013/03/costello_grin_wideweb__470x3082.jpg[/img]

[quote name='CipherWeston' timestamp='1365473923' post='274347'] Funny junk. No. [/quote] >implying the meme originated on funny junk.

[quote name='CipherWeston' timestamp='1365473791' post='274339'] Would've been better if he was ironing an iron. [/quote] [img]http://static2.fjcdn.com/comments/yo+dawg+i+heard+you+belived+in+america+_098d7f55574a2c3393fbbab999c91683.png[/img]

[quote name='ArmisticeAcropolis' timestamp='1365473441' post='274316'] "My eyes are up here" Says the DD Blonde wearing a low cut top so you can see everything but her nips The irony [/quote] [img]http://25.media.tumblr.com/tumblr_m2e8bcNINk1rocyr9o1_500.gif[/img] It's also like triple irony, because women should do the ironing and that's not Iron Woman.

[quote name='Kelarr' timestamp='1365471306' post='274233'] [img]http://gyazo.com/bce3cbc56b846da92ad5738feed35ead.png?1365471014[/img] [/quote] I would enjoy this image more if the stupid bitch wasn't covering her tits with that sign.

[quote name='Buenosan' timestamp='1365400210' post='272443'] and learn a lot from you guys! [/quote] A nebula is an interstellar cloud of dust, hydrogen, helium and other ionized gases. Originally, nebula was a name for any diffuse astronomical object, including galaxies beyond the Milky Way. The Andromeda Galaxy, for instance, was referred to as the Andromeda Nebula (and spiral galaxies in general as "spiral nebulae") before the true nature of galaxies was confirmed in the early 20th century by Vesto Slipher, Edwin Hubble, et. al. Nebulae are often star-forming regions, such as in the Eagle Nebula. This nebula is depicted in one of NASA's most famous images, the "Pillars of Creation". In these regions the formations of gas, dust, and other materials "clump" together to form larger masses, which attract further matter, and eventually will become massive enough to form stars. The remaining materials are then believed to form planets, and other planetary system objects. Around AD 150, Claudius Ptolemaeus (Ptolemy) recorded, in books VII-VIII of his Almagest, five stars that appeared nebulous. He also noted a region of nebulosity between the constellations Ursa Major and Leo that was not associated with any star. The first true nebula, as distinct from a star cluster, was mentioned by the Persian/Muslim astronomer, Abd al-Rahman al-Sufi, in his Book of Fixed Stars (964). He noted "a little cloud" where the Andromeda Galaxy is located.He also cataloged the Omicron Velorum star cluster as a "nebulous star" and other nebulous objects, such as Brocchi's Cluster. The supernova that created the Crab Nebula, the SN 1054, was observed by Arabic and Chinese astronomers in 1054. On November 26, 1610, Nicolas-Claude Fabri de Peiresc discovered the Orion Nebula using a telescope. This nebula was also observed by Johann Baptist Cysat in 1618. However, the first detailed study of the Orion Nebula wouldn't be performed until 1659 by Christian Huygens, who also believed himself to be the first person to discover this nebulosity. In 1715, Edmund Halley published a list of six nebulae. This number steadily increased during the century, with Jean-Philippe de Cheseaux compiling a list of 20 (including eight not previously known) in 1746. From 1751–53, Nicolas Louis de Lacaille cataloged 42 nebulae from the Cape of Good Hope, with most of them being previously unknown. Charles Messier then compiled a catalog of 103 "nebulae" (now called Messier objects, which included what are now known to be galaxies) by 1781; his interest was detecting comets, and these were objects that might be mistaken for them, wasting time. The number of nebulae was then greatly expanded by the efforts of William Herschel and his sister Caroline Herschel. Their Catalogue of One Thousand New Nebulae and Clusters of Stars was published in 1786. A second catalog of a thousand was published in 1789 and the third and final catalog of 510 appeared in 1802. During much of their work, William Herschel believed that these nebulae were merely unresolved clusters of stars. In 1790, however, he discovered a star surrounded by nebulosity and concluded that this was a true nebulosity, rather than a more distant cluster. Beginning in 1864, William Huggins examined the spectra of about 70 nebulae. He found that roughly a third of them had the absorption spectra of a gas. The rest showed a continuous spectrum and thus were thought to consist of a mass of stars. A third category was added in 1912 when Vesto Slipher showed that the spectrum of the nebula that surrounded the star Merope matched the spectra of the Pleiades open cluster. Thus the nebula radiates by reflected star light. In about 1922, following the Great Debate, it had become clear that many "nebulae" were in fact galaxies far from our own. Slipher and Edwin Hubble continued to collect the spectra from many diffuse nebulae, finding 29 that showed emission spectra and 33 had the continuous spectra of star light. In 1922, Hubble announced that nearly all nebulae are associated with stars, and their illumination comes from star light. He also discovered that the emission spectrum nebulae are nearly always associated with stars having spectral classifications of B1 or hotter (including all O-type main sequence stars), while nebulae with continuous spectra appear with cooler stars. Both Hubble and Henry Norris Russell concluded that the nebulae surrounding the hotter stars are transformed in some manner. Many nebulae or stars form from the gravitational collapse of gas in the interstellar medium or ISM. As the material collapses under its own weight, massive stars may form in the center, and their ultraviolet radiation ionizes the surrounding gas, making it visible at optical wavelengths. Examples of these types of nebulae are the Rosette Nebula and the Pelican Nebula. The size of these nebulae, known as HII regions, varies depending on the size of the original cloud of gas. New stars are formed in the nebulas. The formed stars are sometimes known as a young, loose cluster. Some nebulae are formed as the result of supernova explosions, the death throes of massive, short-lived stars. The materials thrown off from the supernova explosion are ionized by the energy and the compact object that it can produce. One of the best examples of this is the Crab Nebula, in Taurus. The supernova event was recorded in the year 1054 and is labelled SN 1054. The compact object that was created after the explosion lies in the center of the Crab Nebula and is a neutron star. Other nebulae may form as planetary nebulae. This is the final stage of a low-mass star's life, like Earth's Sun. Stars with a mass up to 8–10 solar masses evolve into red giants and slowly lose their outer layers during pulsations in their atmospheres. When a star has lost enough material, its temperature increases and the ultraviolet radiation it emits can ionize the surrounding nebula that it has thrown off. The nebula is almost 97% hydrogen and 3% helium, plus trace amounts of other elements.

Too slow, too long, too much time spent on showing customization, should replace shitty audio immediately.

[img]http://www.rottenecards.com/ecards/rottenecard_1541374_4ykxymhvph.png[/img]

It's a huge jump in money and you're bound to get incredibly homesick. You're much more likely to regret the decision shortly down the road. I don't think your costs outweigh your benefits but that's just me. Realistically, you should stay in France and study for far less money.

[quote name='Croix' timestamp='1365279318' post='269701'] Homophobia [/quote] [spoiler][img]http://i591.photobucket.com/albums/ss360/9-esa-1-payasa-6/LESBIANS-3-1.jpg[/img][/spoiler]