by iamlucky13 » Fri Oct 19, 2007 6:26 pm
Electromagnetic radiation (including light) is emitted at some rate by any object warmer than absolute zero. The intensity of the emission depends on the temperature. Interstellar gas is generally very faint, but if it's warmed by a nearby star, it can be brighter, which we often see when a star is hidden behind the gas cloud (so light from the star can't reflect off the gas).
There is much, much more to it, but that's a start. Also, it tends to be specific wavelengths, which is why they talk about the colors assigned to hydrogen, sulfure, and oxygen colors. More about it:
http://csep10.phys.utk.edu/astr162/lect ... ption.html
Electromagnetic radiation (including light) is emitted at some rate by any object warmer than absolute zero. The intensity of the emission depends on the temperature. Interstellar gas is generally very faint, but if it's warmed by a nearby star, it can be brighter, which we often see when a star is hidden behind the gas cloud (so light from the star can't reflect off the gas).
There is much, much more to it, but that's a start. Also, it tends to be specific wavelengths, which is why they talk about the colors assigned to hydrogen, sulfure, and oxygen colors. More about it:
http://csep10.phys.utk.edu/astr162/lect/light/absorption.html