That ' s how it does work on the PS 4 . This may be a feature restricted to the PC version . <| sep |> You ' ll go in , they ' ll go over the basics of the job and give you a company credit card bag . You have to pass the background check , if you haven ' t done jail time then you ' ll get approved . One thing though , at least in NYC , we deliver alcohol tobacco and you ' re too young <| sep |> So you want us to go extinct or what ? ?<| sep |> Maybe you gotta walk up to them or sumptin then shoot . Stupid piece of gawbage <| sep |> I dunno , I ' ve always been told that it ' s pronounced the FED <| sep |> The flame example is misleading you a bit . It is true that hot gas molecules don ' t emit a smooth blackbody spectrum , because the emission spectrum of an object is the product of the ideal blackbody spectrum and its absorption spectrum . Many people forget about the second part , i . e . Kirchhoff ' s law of thermal radiation , and they just assume you are dealing with something close to an ideal blackbody . As a result , hot gases emit spectral lines rather than a continuous spectrum and they can have a variety of colors depending on where those lines cluster . For the flame , the light is also coming from chemiluminescence rather than thermal excitation , but regardless it still emits in sharp lines . But if we look at the sun , we do see more or less a continuous blackbody curve , just like with hot soot . That is because the sun isn ' t a gas , it is a plasma . And plasma absorbs all frequencies . The sun isn ' t a perfect blackbody , because it is partially transparent too . But since the sun is so thick , you only see light from a finite depth range known as the photosphere . The temperature varies a little over the photosphere , so instead of one blackbody curve at one temperature you have to integrate the contribution of different layers up . But the end result is something very close to an ideal blackbody curve at 5777 K . tldr The sun is a plasma , which is a much better blackbody than a gas , so it emits something close to an ideal blackbody curve .